From luminous hot stars to starburst galaxies /:
Luminous hot stars represent the extreme upper mass end of normal stellar evolution. Before exploding as supernovae, they live out their lives of a few million years with prodigious outputs of radiation and stellar winds, dramatically affecting both their evolution and environments. A detailed intro...
Gespeichert in:
| 1. Verfasser: | |
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| Weitere Verfasser: | , |
| Format: | Elektronisch E-Book |
| Sprache: | English |
| Veröffentlicht: |
Cambridge, UK ; New York :
Cambridge University Press,
2008.
|
| Schriftenreihe: | Cambridge astrophysics series ;
45. |
| Schlagworte: | |
| Online-Zugang: | Volltext |
| Zusammenfassung: | Luminous hot stars represent the extreme upper mass end of normal stellar evolution. Before exploding as supernovae, they live out their lives of a few million years with prodigious outputs of radiation and stellar winds, dramatically affecting both their evolution and environments. A detailed introduction to the topic, this book connects the astrophysics of massive stars with the extremes of galaxy evolution represented by starburst phenomena. A thorough discussion of the physical and wind parameters of massive stars is presented. HII galaxies, their connection to starburst galaxies, and the contribution of starburst phenomena to galaxy evolution through superwinds, are explored. The book concludes with the wider cosmological implications, including Population III stars, Lyman break galaxies and gamma-ray bursts, for each of which massive stars are believed to play a crucial role. This book is ideal for graduate students and researchers in astrophysics interested in luminous hot stars and galaxy evolution. |
| Beschreibung: | 1 online resource (xiii, 315 pages) : illustrations |
| Bibliographie: | Includes bibliographical references (pages 294-305) and indexes. |
| ISBN: | 9780511457494 0511457499 0511456182 9780511456183 9780521791342 0521791340 9780511454455 0511454457 9780511455483 0511455488 |
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| 100 | 1 | |a Conti, P. S. |q (Peter S.) |1 https://id.oclc.org/worldcat/entity/E39PCjqykkfPRRCmR7cQQq36Vd |0 http://id.loc.gov/authorities/names/n79028797 | |
| 245 | 1 | 0 | |a From luminous hot stars to starburst galaxies / |c Peter S. Conti, Paul A. Crowther, Claus Leitherer. |
| 260 | |a Cambridge, UK ; |a New York : |b Cambridge University Press, |c 2008. | ||
| 300 | |a 1 online resource (xiii, 315 pages) : |b illustrations | ||
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| 490 | 1 | |a Cambridge astrophysics series ; |v 45 | |
| 504 | |a Includes bibliographical references (pages 294-305) and indexes. | ||
| 588 | 0 | |a Print version record. | |
| 505 | 0 | 0 | |g 1.1 |t Motivation |g 1 -- |g 1.2 |t Observed properties |g 1 -- |g 1.3 |t Stellar atmospheres |g 5 -- |g 1.4 |t Stellar winds |g 5 -- |g 1.5 |t Evolution of single stars |g 7 -- |g 1.6 |t Binaries |g 9 -- |g 1.7 |t Birth of massive stars and star clusters |g 10 -- |g 1.8 |t The interstellar environment |g 11 -- |g 1.9 |t From GHII regions to starburst galaxies |g 12 -- |g 1.10 |t Starburst phenomena |g 14 -- |g 1.11 |t Cosmological implications |g 15 -- |g 2 |t Observed properties |g 17 -- |g 2.1 |t Apparent and absolute magnitudes |g 17 -- |g 2.2 |t Distances |g 19 -- |g 2.3 |t Massive stars in Local Group galaxies |g 21 -- |g 2.4 |t Spectral classification |g 35 -- |g 2.5 |t Observations of rotation and magnetic fields |g 45 -- |g 3 |t Stellar atmospheres |g 49 -- |g 3.1 |t LTE atmospheres |g 49 -- |g 3.2 |t Non-LTE atmospheres |g 50 -- |g 3.3 |t Surface gravities and masses |g 61 -- |g 3.4 |t Surface composition |g 62 -- |g 4 |t Stellar winds |g 67 -- |g 4.1 |t Radiation pressure |g 67 -- |g 4.2 |t Wind velocities |g 74 -- |g 4.3 |t Mass-loss rates |g 79 -- |g 4.4 |t Structure and clumping |g 90 -- |g 4.5 |t Influence of stellar rotation |g 95 -- |g 5 |t Evolution of single stars |g 99 -- |g 5.1 |t Nucleosynthesis |g 99 -- |g 5.2 |t Evolution to a red supergiant |g 102 -- |g 5.3 |t Evolution to the Wolf-Rayet stage |g 107 -- |g 5.4 |t Rotation and mass-loss |g 111 -- |g 5.5 |t Magnetic massive stars |g 115 -- |g 5.6 |t Core-collapse supernovae |g 116 -- |g 6 |t Binaries |g 129 -- |g 6.1 |t Massive binary frequency |g 129 -- |g 6.2 |t Binary masses |g 130 -- |g 6.3 |t Close binary evolution |g 133 -- |g 6.4 |t Interacting stellar winds |g 146 -- |g 6.5 |t Dust formation in WC stars |g 149 -- |g 7 |t Birth of massive stars and star clusters |g 154 -- |g 7.1 |t Natal precursors of OB stars |g 155 -- |g 7.2 |t The initial mass function |g 163 -- |g 7.3 |t Formation of high-mass stars |g 167 -- |g 7.4 |t Massive stellar clusters |g 170 -- |g 8 |t The interstellar environment |g 180 -- |g 8.1 |t Interstellar dust |g 180 -- |g 8.2 |t Ionized hydrogen regions |g 184 -- |g 8.3 |t Wind blown bubbles |g 187 -- |g 8.4 |t Ejecta nebulae around LBVs and W-R stars |g 192 -- |g 9 |t From giant HII regions to HII galaxies |g 197 -- |g 9.1 |t Giant HII regions: definition and structural parameters |g 197 -- |g 9.2 |t 30 Doradus -- the Rosetta Stone |g 200 -- |g 9.3 |t Stellar population diagnostics |g 208 -- |g 9.4 |t HII galaxies: stellar content and relation to starbursts |g 219 -- |g 10 |t Starburst phenomena |g 229 -- |g 10.1 |t Definition of a starburst |g 229 -- |g 10.2 |t The starburst IMF |g 231 -- |g 10.3 |t The evolution of starbursts |g 241 -- |g 10.4 |t Starburst-driven superwinds |g 250 -- |g 10.5 |t The starburst-AGN connection |g 255 -- |g 11 |t Cosmological implications |g 266 -- |g 11.1 |t Population III stars |g 266 -- |g 11.2 |t Lyman-break galaxies |g 272 -- |g 11.3 |t Massive stars and cosmic abundances |g 280 -- |g 11.4 |t Gamma ray bursts |g 287. |
| 520 | |a Luminous hot stars represent the extreme upper mass end of normal stellar evolution. Before exploding as supernovae, they live out their lives of a few million years with prodigious outputs of radiation and stellar winds, dramatically affecting both their evolution and environments. A detailed introduction to the topic, this book connects the astrophysics of massive stars with the extremes of galaxy evolution represented by starburst phenomena. A thorough discussion of the physical and wind parameters of massive stars is presented. HII galaxies, their connection to starburst galaxies, and the contribution of starburst phenomena to galaxy evolution through superwinds, are explored. The book concludes with the wider cosmological implications, including Population III stars, Lyman break galaxies and gamma-ray bursts, for each of which massive stars are believed to play a crucial role. This book is ideal for graduate students and researchers in astrophysics interested in luminous hot stars and galaxy evolution. | ||
| 650 | 0 | |a Starbursts. |0 http://id.loc.gov/authorities/subjects/sh92001132 | |
| 650 | 0 | |a Gamma ray bursts. |0 http://id.loc.gov/authorities/subjects/sh85052983 | |
| 650 | 0 | |a Stars |x Evolution. |0 http://id.loc.gov/authorities/subjects/sh85127430 | |
| 650 | 0 | |a Stellar winds. |0 http://id.loc.gov/authorities/subjects/sh88000835 | |
| 650 | 6 | |a Sursauts de formation d'étoiles. | |
| 650 | 6 | |a Sursauts gamma. | |
| 650 | 6 | |a Étoiles |x Évolution. | |
| 650 | 6 | |a Vents stellaires. | |
| 650 | 7 | |a SCIENCE |x Cosmology. |2 bisacsh | |
| 650 | 7 | |a Gamma ray bursts |2 fast | |
| 650 | 7 | |a Starbursts |2 fast | |
| 650 | 7 | |a Stars |x Evolution |2 fast | |
| 650 | 7 | |a Stellar winds |2 fast | |
| 700 | 1 | |a Crowther, Paul A. |0 http://id.loc.gov/authorities/names/no2003008784 | |
| 700 | 1 | |a Leitherer, Claus. |0 http://id.loc.gov/authorities/names/nr91025722 | |
| 776 | 0 | 8 | |i Print version: |a Conti, P.S. (Peter S.). |t From luminous hot stars to starburst galaxies. |d Cambridge, UK ; New York : Cambridge University Press, 2008 |z 9780521791342 |z 0521791340 |w (DLC) 2008031554 |w (OCoLC)221147294 |
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Datensatz im Suchindex
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| _version_ | 1816881687481548800 |
| adam_text | |
| any_adam_object | |
| author | Conti, P. S. (Peter S.) |
| author2 | Crowther, Paul A. Leitherer, Claus |
| author2_role | |
| author2_variant | p a c pa pac c l cl |
| author_GND | http://id.loc.gov/authorities/names/n79028797 http://id.loc.gov/authorities/names/no2003008784 http://id.loc.gov/authorities/names/nr91025722 |
| author_facet | Conti, P. S. (Peter S.) Crowther, Paul A. Leitherer, Claus |
| author_role | |
| author_sort | Conti, P. S. |
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| building | Verbundindex |
| bvnumber | localFWS |
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| collection | ZDB-4-EBA |
| contents | Motivation Observed properties Stellar atmospheres Stellar winds Evolution of single stars Binaries Birth of massive stars and star clusters The interstellar environment From GHII regions to starburst galaxies Starburst phenomena Cosmological implications Apparent and absolute magnitudes Distances Massive stars in Local Group galaxies Spectral classification Observations of rotation and magnetic fields LTE atmospheres Non-LTE atmospheres Surface gravities and masses Surface composition Radiation pressure Wind velocities Mass-loss rates Structure and clumping Influence of stellar rotation Nucleosynthesis Evolution to a red supergiant Evolution to the Wolf-Rayet stage Rotation and mass-loss Magnetic massive stars Core-collapse supernovae Massive binary frequency Binary masses Close binary evolution Interacting stellar winds Dust formation in WC stars Natal precursors of OB stars The initial mass function Formation of high-mass stars Massive stellar clusters Interstellar dust Ionized hydrogen regions Wind blown bubbles Ejecta nebulae around LBVs and W-R stars From giant HII regions to HII galaxies Giant HII regions: definition and structural parameters 30 Doradus -- the Rosetta Stone Stellar population diagnostics HII galaxies: stellar content and relation to starbursts Definition of a starburst The starburst IMF The evolution of starbursts Starburst-driven superwinds The starburst-AGN connection Population III stars Lyman-break galaxies Massive stars and cosmic abundances Gamma ray bursts |
| ctrlnum | (OCoLC)311079929 |
| dewey-full | 523.1/125 |
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| dewey-ones | 523 - Specific celestial bodies and phenomena |
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| dewey-sort | 3523.1 3125 |
| dewey-tens | 520 - Astronomy and allied sciences |
| discipline | Physik |
| format | Electronic eBook |
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composition</subfield><subfield code="g">62 --</subfield><subfield code="g">4</subfield><subfield code="t">Stellar winds</subfield><subfield code="g">67 --</subfield><subfield code="g">4.1</subfield><subfield code="t">Radiation pressure</subfield><subfield code="g">67 --</subfield><subfield code="g">4.2</subfield><subfield code="t">Wind velocities</subfield><subfield code="g">74 --</subfield><subfield code="g">4.3</subfield><subfield code="t">Mass-loss rates</subfield><subfield code="g">79 --</subfield><subfield code="g">4.4</subfield><subfield code="t">Structure and clumping</subfield><subfield code="g">90 --</subfield><subfield code="g">4.5</subfield><subfield code="t">Influence of stellar rotation</subfield><subfield code="g">95 --</subfield><subfield code="g">5</subfield><subfield code="t">Evolution of single stars</subfield><subfield code="g">99 --</subfield><subfield code="g">5.1</subfield><subfield code="t">Nucleosynthesis</subfield><subfield code="g">99 --</subfield><subfield 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code="t">Close binary evolution</subfield><subfield code="g">133 --</subfield><subfield code="g">6.4</subfield><subfield code="t">Interacting stellar winds</subfield><subfield code="g">146 --</subfield><subfield code="g">6.5</subfield><subfield code="t">Dust formation in WC stars</subfield><subfield code="g">149 --</subfield><subfield code="g">7</subfield><subfield code="t">Birth of massive stars and star clusters</subfield><subfield code="g">154 --</subfield><subfield code="g">7.1</subfield><subfield code="t">Natal precursors of OB stars</subfield><subfield code="g">155 --</subfield><subfield code="g">7.2</subfield><subfield code="t">The initial mass function</subfield><subfield code="g">163 --</subfield><subfield code="g">7.3</subfield><subfield code="t">Formation of high-mass stars</subfield><subfield code="g">167 --</subfield><subfield code="g">7.4</subfield><subfield code="t">Massive stellar clusters</subfield><subfield code="g">170 --</subfield><subfield code="g">8</subfield><subfield code="t">The interstellar environment</subfield><subfield code="g">180 --</subfield><subfield code="g">8.1</subfield><subfield code="t">Interstellar dust</subfield><subfield code="g">180 --</subfield><subfield code="g">8.2</subfield><subfield code="t">Ionized hydrogen regions</subfield><subfield code="g">184 --</subfield><subfield code="g">8.3</subfield><subfield code="t">Wind blown bubbles</subfield><subfield code="g">187 --</subfield><subfield code="g">8.4</subfield><subfield code="t">Ejecta nebulae around LBVs and W-R stars</subfield><subfield code="g">192 --</subfield><subfield code="g">9</subfield><subfield code="t">From giant HII regions to HII galaxies</subfield><subfield code="g">197 --</subfield><subfield code="g">9.1</subfield><subfield code="t">Giant HII regions: definition and structural parameters</subfield><subfield code="g">197 --</subfield><subfield code="g">9.2</subfield><subfield code="t">30 Doradus -- the Rosetta Stone</subfield><subfield code="g">200 --</subfield><subfield code="g">9.3</subfield><subfield code="t">Stellar population diagnostics</subfield><subfield code="g">208 --</subfield><subfield code="g">9.4</subfield><subfield code="t">HII galaxies: stellar content and relation to starbursts</subfield><subfield code="g">219 --</subfield><subfield code="g">10</subfield><subfield code="t">Starburst phenomena</subfield><subfield code="g">229 --</subfield><subfield code="g">10.1</subfield><subfield code="t">Definition of a starburst</subfield><subfield code="g">229 --</subfield><subfield code="g">10.2</subfield><subfield code="t">The starburst IMF</subfield><subfield code="g">231 --</subfield><subfield code="g">10.3</subfield><subfield code="t">The evolution of starbursts</subfield><subfield code="g">241 --</subfield><subfield code="g">10.4</subfield><subfield code="t">Starburst-driven superwinds</subfield><subfield code="g">250 --</subfield><subfield code="g">10.5</subfield><subfield code="t">The starburst-AGN connection</subfield><subfield code="g">255 --</subfield><subfield code="g">11</subfield><subfield code="t">Cosmological implications</subfield><subfield code="g">266 --</subfield><subfield code="g">11.1</subfield><subfield code="t">Population III stars</subfield><subfield code="g">266 --</subfield><subfield code="g">11.2</subfield><subfield code="t">Lyman-break galaxies</subfield><subfield code="g">272 --</subfield><subfield code="g">11.3</subfield><subfield code="t">Massive stars and cosmic abundances</subfield><subfield code="g">280 --</subfield><subfield code="g">11.4</subfield><subfield code="t">Gamma ray bursts</subfield><subfield code="g">287.</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Luminous hot stars represent the extreme upper mass end of normal stellar evolution. Before exploding as supernovae, they live out their lives of a few million years with prodigious outputs of radiation and stellar winds, dramatically affecting both their evolution and environments. A detailed introduction to the topic, this book connects the astrophysics of massive stars with the extremes of galaxy evolution represented by starburst phenomena. A thorough discussion of the physical and wind parameters of massive stars is presented. HII galaxies, their connection to starburst galaxies, and the contribution of starburst phenomena to galaxy evolution through superwinds, are explored. The book concludes with the wider cosmological implications, including Population III stars, Lyman break galaxies and gamma-ray bursts, for each of which massive stars are believed to play a crucial role. This book is ideal for graduate students and researchers in astrophysics interested in luminous hot stars and galaxy evolution.</subfield></datafield><datafield tag="650" ind1=" " ind2="0"><subfield code="a">Starbursts.</subfield><subfield code="0">http://id.loc.gov/authorities/subjects/sh92001132</subfield></datafield><datafield tag="650" ind1=" " ind2="0"><subfield code="a">Gamma ray bursts.</subfield><subfield code="0">http://id.loc.gov/authorities/subjects/sh85052983</subfield></datafield><datafield tag="650" ind1=" " ind2="0"><subfield code="a">Stars</subfield><subfield code="x">Evolution.</subfield><subfield code="0">http://id.loc.gov/authorities/subjects/sh85127430</subfield></datafield><datafield tag="650" ind1=" " ind2="0"><subfield code="a">Stellar winds.</subfield><subfield code="0">http://id.loc.gov/authorities/subjects/sh88000835</subfield></datafield><datafield tag="650" ind1=" " ind2="6"><subfield code="a">Sursauts de formation d'étoiles.</subfield></datafield><datafield tag="650" ind1=" " ind2="6"><subfield code="a">Sursauts gamma.</subfield></datafield><datafield tag="650" ind1=" " ind2="6"><subfield code="a">Étoiles</subfield><subfield code="x">Évolution.</subfield></datafield><datafield tag="650" ind1=" " ind2="6"><subfield code="a">Vents stellaires.</subfield></datafield><datafield tag="650" ind1=" " ind2="7"><subfield code="a">SCIENCE</subfield><subfield code="x">Cosmology.</subfield><subfield code="2">bisacsh</subfield></datafield><datafield tag="650" ind1=" " ind2="7"><subfield code="a">Gamma ray bursts</subfield><subfield code="2">fast</subfield></datafield><datafield tag="650" ind1=" " ind2="7"><subfield code="a">Starbursts</subfield><subfield code="2">fast</subfield></datafield><datafield tag="650" ind1=" " ind2="7"><subfield code="a">Stars</subfield><subfield code="x">Evolution</subfield><subfield code="2">fast</subfield></datafield><datafield tag="650" ind1=" " ind2="7"><subfield code="a">Stellar winds</subfield><subfield code="2">fast</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Crowther, Paul A.</subfield><subfield code="0">http://id.loc.gov/authorities/names/no2003008784</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Leitherer, Claus.</subfield><subfield code="0">http://id.loc.gov/authorities/names/nr91025722</subfield></datafield><datafield tag="776" ind1="0" ind2="8"><subfield code="i">Print version:</subfield><subfield code="a">Conti, P.S. 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| id | ZDB-4-EBA-ocn311079929 |
| illustrated | Illustrated |
| indexdate | 2024-11-27T13:16:41Z |
| institution | BVB |
| isbn | 9780511457494 0511457499 0511456182 9780511456183 9780521791342 0521791340 9780511454455 0511454457 9780511455483 0511455488 |
| language | English |
| oclc_num | 311079929 |
| open_access_boolean | |
| owner | MAIN DE-863 DE-BY-FWS |
| owner_facet | MAIN DE-863 DE-BY-FWS |
| physical | 1 online resource (xiii, 315 pages) : illustrations |
| psigel | ZDB-4-EBA |
| publishDate | 2008 |
| publishDateSearch | 2008 |
| publishDateSort | 2008 |
| publisher | Cambridge University Press, |
| record_format | marc |
| series | Cambridge astrophysics series ; |
| series2 | Cambridge astrophysics series ; |
| spelling | Conti, P. S. (Peter S.) https://id.oclc.org/worldcat/entity/E39PCjqykkfPRRCmR7cQQq36Vd http://id.loc.gov/authorities/names/n79028797 From luminous hot stars to starburst galaxies / Peter S. Conti, Paul A. Crowther, Claus Leitherer. Cambridge, UK ; New York : Cambridge University Press, 2008. 1 online resource (xiii, 315 pages) : illustrations text txt rdacontent computer c rdamedia online resource cr rdacarrier Cambridge astrophysics series ; 45 Includes bibliographical references (pages 294-305) and indexes. Print version record. 1.1 Motivation 1 -- 1.2 Observed properties 1 -- 1.3 Stellar atmospheres 5 -- 1.4 Stellar winds 5 -- 1.5 Evolution of single stars 7 -- 1.6 Binaries 9 -- 1.7 Birth of massive stars and star clusters 10 -- 1.8 The interstellar environment 11 -- 1.9 From GHII regions to starburst galaxies 12 -- 1.10 Starburst phenomena 14 -- 1.11 Cosmological implications 15 -- 2 Observed properties 17 -- 2.1 Apparent and absolute magnitudes 17 -- 2.2 Distances 19 -- 2.3 Massive stars in Local Group galaxies 21 -- 2.4 Spectral classification 35 -- 2.5 Observations of rotation and magnetic fields 45 -- 3 Stellar atmospheres 49 -- 3.1 LTE atmospheres 49 -- 3.2 Non-LTE atmospheres 50 -- 3.3 Surface gravities and masses 61 -- 3.4 Surface composition 62 -- 4 Stellar winds 67 -- 4.1 Radiation pressure 67 -- 4.2 Wind velocities 74 -- 4.3 Mass-loss rates 79 -- 4.4 Structure and clumping 90 -- 4.5 Influence of stellar rotation 95 -- 5 Evolution of single stars 99 -- 5.1 Nucleosynthesis 99 -- 5.2 Evolution to a red supergiant 102 -- 5.3 Evolution to the Wolf-Rayet stage 107 -- 5.4 Rotation and mass-loss 111 -- 5.5 Magnetic massive stars 115 -- 5.6 Core-collapse supernovae 116 -- 6 Binaries 129 -- 6.1 Massive binary frequency 129 -- 6.2 Binary masses 130 -- 6.3 Close binary evolution 133 -- 6.4 Interacting stellar winds 146 -- 6.5 Dust formation in WC stars 149 -- 7 Birth of massive stars and star clusters 154 -- 7.1 Natal precursors of OB stars 155 -- 7.2 The initial mass function 163 -- 7.3 Formation of high-mass stars 167 -- 7.4 Massive stellar clusters 170 -- 8 The interstellar environment 180 -- 8.1 Interstellar dust 180 -- 8.2 Ionized hydrogen regions 184 -- 8.3 Wind blown bubbles 187 -- 8.4 Ejecta nebulae around LBVs and W-R stars 192 -- 9 From giant HII regions to HII galaxies 197 -- 9.1 Giant HII regions: definition and structural parameters 197 -- 9.2 30 Doradus -- the Rosetta Stone 200 -- 9.3 Stellar population diagnostics 208 -- 9.4 HII galaxies: stellar content and relation to starbursts 219 -- 10 Starburst phenomena 229 -- 10.1 Definition of a starburst 229 -- 10.2 The starburst IMF 231 -- 10.3 The evolution of starbursts 241 -- 10.4 Starburst-driven superwinds 250 -- 10.5 The starburst-AGN connection 255 -- 11 Cosmological implications 266 -- 11.1 Population III stars 266 -- 11.2 Lyman-break galaxies 272 -- 11.3 Massive stars and cosmic abundances 280 -- 11.4 Gamma ray bursts 287. Luminous hot stars represent the extreme upper mass end of normal stellar evolution. Before exploding as supernovae, they live out their lives of a few million years with prodigious outputs of radiation and stellar winds, dramatically affecting both their evolution and environments. A detailed introduction to the topic, this book connects the astrophysics of massive stars with the extremes of galaxy evolution represented by starburst phenomena. A thorough discussion of the physical and wind parameters of massive stars is presented. HII galaxies, their connection to starburst galaxies, and the contribution of starburst phenomena to galaxy evolution through superwinds, are explored. The book concludes with the wider cosmological implications, including Population III stars, Lyman break galaxies and gamma-ray bursts, for each of which massive stars are believed to play a crucial role. This book is ideal for graduate students and researchers in astrophysics interested in luminous hot stars and galaxy evolution. Starbursts. http://id.loc.gov/authorities/subjects/sh92001132 Gamma ray bursts. http://id.loc.gov/authorities/subjects/sh85052983 Stars Evolution. http://id.loc.gov/authorities/subjects/sh85127430 Stellar winds. http://id.loc.gov/authorities/subjects/sh88000835 Sursauts de formation d'étoiles. Sursauts gamma. Étoiles Évolution. Vents stellaires. SCIENCE Cosmology. bisacsh Gamma ray bursts fast Starbursts fast Stars Evolution fast Stellar winds fast Crowther, Paul A. http://id.loc.gov/authorities/names/no2003008784 Leitherer, Claus. http://id.loc.gov/authorities/names/nr91025722 Print version: Conti, P.S. (Peter S.). From luminous hot stars to starburst galaxies. Cambridge, UK ; New York : Cambridge University Press, 2008 9780521791342 0521791340 (DLC) 2008031554 (OCoLC)221147294 Cambridge astrophysics series ; 45. http://id.loc.gov/authorities/names/n42034737 FWS01 ZDB-4-EBA FWS_PDA_EBA https://search.ebscohost.com/login.aspx?direct=true&scope=site&db=nlebk&AN=259193 Volltext |
| spellingShingle | Conti, P. S. (Peter S.) From luminous hot stars to starburst galaxies / Cambridge astrophysics series ; Motivation Observed properties Stellar atmospheres Stellar winds Evolution of single stars Binaries Birth of massive stars and star clusters The interstellar environment From GHII regions to starburst galaxies Starburst phenomena Cosmological implications Apparent and absolute magnitudes Distances Massive stars in Local Group galaxies Spectral classification Observations of rotation and magnetic fields LTE atmospheres Non-LTE atmospheres Surface gravities and masses Surface composition Radiation pressure Wind velocities Mass-loss rates Structure and clumping Influence of stellar rotation Nucleosynthesis Evolution to a red supergiant Evolution to the Wolf-Rayet stage Rotation and mass-loss Magnetic massive stars Core-collapse supernovae Massive binary frequency Binary masses Close binary evolution Interacting stellar winds Dust formation in WC stars Natal precursors of OB stars The initial mass function Formation of high-mass stars Massive stellar clusters Interstellar dust Ionized hydrogen regions Wind blown bubbles Ejecta nebulae around LBVs and W-R stars From giant HII regions to HII galaxies Giant HII regions: definition and structural parameters 30 Doradus -- the Rosetta Stone Stellar population diagnostics HII galaxies: stellar content and relation to starbursts Definition of a starburst The starburst IMF The evolution of starbursts Starburst-driven superwinds The starburst-AGN connection Population III stars Lyman-break galaxies Massive stars and cosmic abundances Gamma ray bursts Starbursts. http://id.loc.gov/authorities/subjects/sh92001132 Gamma ray bursts. http://id.loc.gov/authorities/subjects/sh85052983 Stars Evolution. http://id.loc.gov/authorities/subjects/sh85127430 Stellar winds. http://id.loc.gov/authorities/subjects/sh88000835 Sursauts de formation d'étoiles. Sursauts gamma. Étoiles Évolution. Vents stellaires. SCIENCE Cosmology. bisacsh Gamma ray bursts fast Starbursts fast Stars Evolution fast Stellar winds fast |
| subject_GND | http://id.loc.gov/authorities/subjects/sh92001132 http://id.loc.gov/authorities/subjects/sh85052983 http://id.loc.gov/authorities/subjects/sh85127430 http://id.loc.gov/authorities/subjects/sh88000835 |
| title | From luminous hot stars to starburst galaxies / |
| title_alt | Motivation Observed properties Stellar atmospheres Stellar winds Evolution of single stars Binaries Birth of massive stars and star clusters The interstellar environment From GHII regions to starburst galaxies Starburst phenomena Cosmological implications Apparent and absolute magnitudes Distances Massive stars in Local Group galaxies Spectral classification Observations of rotation and magnetic fields LTE atmospheres Non-LTE atmospheres Surface gravities and masses Surface composition Radiation pressure Wind velocities Mass-loss rates Structure and clumping Influence of stellar rotation Nucleosynthesis Evolution to a red supergiant Evolution to the Wolf-Rayet stage Rotation and mass-loss Magnetic massive stars Core-collapse supernovae Massive binary frequency Binary masses Close binary evolution Interacting stellar winds Dust formation in WC stars Natal precursors of OB stars The initial mass function Formation of high-mass stars Massive stellar clusters Interstellar dust Ionized hydrogen regions Wind blown bubbles Ejecta nebulae around LBVs and W-R stars From giant HII regions to HII galaxies Giant HII regions: definition and structural parameters 30 Doradus -- the Rosetta Stone Stellar population diagnostics HII galaxies: stellar content and relation to starbursts Definition of a starburst The starburst IMF The evolution of starbursts Starburst-driven superwinds The starburst-AGN connection Population III stars Lyman-break galaxies Massive stars and cosmic abundances Gamma ray bursts |
| title_auth | From luminous hot stars to starburst galaxies / |
| title_exact_search | From luminous hot stars to starburst galaxies / |
| title_full | From luminous hot stars to starburst galaxies / Peter S. Conti, Paul A. Crowther, Claus Leitherer. |
| title_fullStr | From luminous hot stars to starburst galaxies / Peter S. Conti, Paul A. Crowther, Claus Leitherer. |
| title_full_unstemmed | From luminous hot stars to starburst galaxies / Peter S. Conti, Paul A. Crowther, Claus Leitherer. |
| title_short | From luminous hot stars to starburst galaxies / |
| title_sort | from luminous hot stars to starburst galaxies |
| topic | Starbursts. http://id.loc.gov/authorities/subjects/sh92001132 Gamma ray bursts. http://id.loc.gov/authorities/subjects/sh85052983 Stars Evolution. http://id.loc.gov/authorities/subjects/sh85127430 Stellar winds. http://id.loc.gov/authorities/subjects/sh88000835 Sursauts de formation d'étoiles. Sursauts gamma. Étoiles Évolution. Vents stellaires. SCIENCE Cosmology. bisacsh Gamma ray bursts fast Starbursts fast Stars Evolution fast Stellar winds fast |
| topic_facet | Starbursts. Gamma ray bursts. Stars Evolution. Stellar winds. Sursauts de formation d'étoiles. Sursauts gamma. Étoiles Évolution. Vents stellaires. SCIENCE Cosmology. Gamma ray bursts Starbursts Stars Evolution Stellar winds |
| url | https://search.ebscohost.com/login.aspx?direct=true&scope=site&db=nlebk&AN=259193 |
| work_keys_str_mv | AT contips fromluminoushotstarstostarburstgalaxies AT crowtherpaula fromluminoushotstarstostarburstgalaxies AT leithererclaus fromluminoushotstarstostarburstgalaxies |