Stellar evolution physics, Volume 1, Physical processes in stellar interiors:
This text describes the microscopic physics operating in stars and demonstrates how stars respond from formation, through hydrogen-burning phases, up to the onset of helium burning. Intended for beginning graduate students and senior undergraduates with a solid background in physics, it illustrates...
Gespeichert in:
| 1. Verfasser: | |
|---|---|
| Format: | Elektronisch E-Book |
| Sprache: | English |
| Veröffentlicht: |
Cambridge
Cambridge University Press
2013
|
| Schlagworte: | |
| Online-Zugang: | BSB01 FHN01 Volltext |
| Zusammenfassung: | This text describes the microscopic physics operating in stars and demonstrates how stars respond from formation, through hydrogen-burning phases, up to the onset of helium burning. Intended for beginning graduate students and senior undergraduates with a solid background in physics, it illustrates the intricate interplay between the microscopic physical processes and the stars' macroscopic responses. The volume starts with the gravitationally contracting phase which carries the star from formation to the core hydrogen-burning main sequence, through the main sequence phase, through shell hydrogen-burning phases as a red giant, up to the onset of core helium burning. Particular emphasis is placed on describing the gravothermal responses of stars to nuclear transformations in the interior and energy loss from the surface, responses which express the very essence of stellar evolution. The volume is replete with many illustrations and detailed numerical solutions to prepare the reader to program and calculate evolutionary models |
| Beschreibung: | Title from publisher's bibliographic system (viewed on 05 Oct 2015) |
| Beschreibung: | 1 online resource (xvi, 890 pages) |
| ISBN: | 9781139061223 |
| DOI: | 10.1017/CBO9781139061223 |
Internformat
MARC
| LEADER | 00000nmm a2200000zc 4500 | ||
|---|---|---|---|
| 001 | BV043945930 | ||
| 003 | DE-604 | ||
| 005 | 00000000000000.0 | ||
| 007 | cr|uuu---uuuuu | ||
| 008 | 161206s2013 |||| o||u| ||||||eng d | ||
| 020 | |a 9781139061223 |c Online |9 978-1-139-06122-3 | ||
| 024 | 7 | |a 10.1017/CBO9781139061223 |2 doi | |
| 035 | |a (ZDB-20-CBO)CR9781139061223 | ||
| 035 | |a (OCoLC)874382789 | ||
| 035 | |a (DE-599)BVBBV043945930 | ||
| 040 | |a DE-604 |b ger |e rda | ||
| 041 | 0 | |a eng | |
| 049 | |a DE-12 |a DE-92 | ||
| 082 | 0 | |a 523.8/8 |2 23 | |
| 100 | 1 | |a Iben, Icko |d 1931- |e Verfasser |4 aut | |
| 245 | 1 | 0 | |a Stellar evolution physics, Volume 1, Physical processes in stellar interiors |c Icko Iben |
| 264 | 1 | |a Cambridge |b Cambridge University Press |c 2013 | |
| 300 | |a 1 online resource (xvi, 890 pages) | ||
| 336 | |b txt |2 rdacontent | ||
| 337 | |b c |2 rdamedia | ||
| 338 | |b cr |2 rdacarrier | ||
| 500 | |a Title from publisher's bibliographic system (viewed on 05 Oct 2015) | ||
| 520 | |a This text describes the microscopic physics operating in stars and demonstrates how stars respond from formation, through hydrogen-burning phases, up to the onset of helium burning. Intended for beginning graduate students and senior undergraduates with a solid background in physics, it illustrates the intricate interplay between the microscopic physical processes and the stars' macroscopic responses. The volume starts with the gravitationally contracting phase which carries the star from formation to the core hydrogen-burning main sequence, through the main sequence phase, through shell hydrogen-burning phases as a red giant, up to the onset of core helium burning. Particular emphasis is placed on describing the gravothermal responses of stars to nuclear transformations in the interior and energy loss from the surface, responses which express the very essence of stellar evolution. The volume is replete with many illustrations and detailed numerical solutions to prepare the reader to program and calculate evolutionary models | ||
| 650 | 4 | |a Stars / Evolution | |
| 650 | 4 | |a Stellar dynamics | |
| 650 | 0 | 7 | |a Heliumbrennen |0 (DE-588)4778553-6 |2 gnd |9 rswk-swf |
| 650 | 0 | 7 | |a Sternentwicklung |0 (DE-588)4057365-5 |2 gnd |9 rswk-swf |
| 650 | 0 | 7 | |a Wasserstoffbrennen |0 (DE-588)4529649-2 |2 gnd |9 rswk-swf |
| 689 | 0 | 0 | |a Sternentwicklung |0 (DE-588)4057365-5 |D s |
| 689 | 0 | 1 | |a Wasserstoffbrennen |0 (DE-588)4529649-2 |D s |
| 689 | 0 | 2 | |a Heliumbrennen |0 (DE-588)4778553-6 |D s |
| 689 | 0 | |5 DE-604 | |
| 776 | 0 | 8 | |i Erscheint auch als |n Druckausgabe |z 978-1-107-01656-9 |
| 856 | 4 | 0 | |u https://doi.org/10.1017/CBO9781139061223 |x Verlag |z URL des Erstveröffentlichers |3 Volltext |
| 912 | |a ZDB-20-CBO | ||
| 999 | |a oai:aleph.bib-bvb.de:BVB01-029354901 | ||
| 966 | e | |u https://doi.org/10.1017/CBO9781139061223 |l BSB01 |p ZDB-20-CBO |q BSB_PDA_CBO |x Verlag |3 Volltext | |
| 966 | e | |u https://doi.org/10.1017/CBO9781139061223 |l FHN01 |p ZDB-20-CBO |q FHN_PDA_CBO |x Verlag |3 Volltext | |
Datensatz im Suchindex
| _version_ | 1804176892637478912 |
|---|---|
| any_adam_object | |
| author | Iben, Icko 1931- |
| author_facet | Iben, Icko 1931- |
| author_role | aut |
| author_sort | Iben, Icko 1931- |
| author_variant | i i ii |
| building | Verbundindex |
| bvnumber | BV043945930 |
| collection | ZDB-20-CBO |
| ctrlnum | (ZDB-20-CBO)CR9781139061223 (OCoLC)874382789 (DE-599)BVBBV043945930 |
| dewey-full | 523.8/8 |
| dewey-hundreds | 500 - Natural sciences and mathematics |
| dewey-ones | 523 - Specific celestial bodies and phenomena |
| dewey-raw | 523.8/8 |
| dewey-search | 523.8/8 |
| dewey-sort | 3523.8 18 |
| dewey-tens | 520 - Astronomy and allied sciences |
| discipline | Physik |
| doi_str_mv | 10.1017/CBO9781139061223 |
| format | Electronic eBook |
| fullrecord | <?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>02926nmm a2200481zc 4500</leader><controlfield tag="001">BV043945930</controlfield><controlfield tag="003">DE-604</controlfield><controlfield tag="005">00000000000000.0</controlfield><controlfield tag="007">cr|uuu---uuuuu</controlfield><controlfield tag="008">161206s2013 |||| o||u| ||||||eng d</controlfield><datafield tag="020" ind1=" " ind2=" "><subfield code="a">9781139061223</subfield><subfield code="c">Online</subfield><subfield code="9">978-1-139-06122-3</subfield></datafield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1017/CBO9781139061223</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(ZDB-20-CBO)CR9781139061223</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(OCoLC)874382789</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-599)BVBBV043945930</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-604</subfield><subfield code="b">ger</subfield><subfield code="e">rda</subfield></datafield><datafield tag="041" ind1="0" ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="049" ind1=" " ind2=" "><subfield code="a">DE-12</subfield><subfield code="a">DE-92</subfield></datafield><datafield tag="082" ind1="0" ind2=" "><subfield code="a">523.8/8</subfield><subfield code="2">23</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Iben, Icko</subfield><subfield code="d">1931-</subfield><subfield code="e">Verfasser</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Stellar evolution physics, Volume 1, Physical processes in stellar interiors</subfield><subfield code="c">Icko Iben</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="a">Cambridge</subfield><subfield code="b">Cambridge University Press</subfield><subfield code="c">2013</subfield></datafield><datafield tag="300" ind1=" " ind2=" "><subfield code="a">1 online resource (xvi, 890 pages)</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="b">c</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="b">cr</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="500" ind1=" " ind2=" "><subfield code="a">Title from publisher's bibliographic system (viewed on 05 Oct 2015)</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">This text describes the microscopic physics operating in stars and demonstrates how stars respond from formation, through hydrogen-burning phases, up to the onset of helium burning. Intended for beginning graduate students and senior undergraduates with a solid background in physics, it illustrates the intricate interplay between the microscopic physical processes and the stars' macroscopic responses. The volume starts with the gravitationally contracting phase which carries the star from formation to the core hydrogen-burning main sequence, through the main sequence phase, through shell hydrogen-burning phases as a red giant, up to the onset of core helium burning. Particular emphasis is placed on describing the gravothermal responses of stars to nuclear transformations in the interior and energy loss from the surface, responses which express the very essence of stellar evolution. The volume is replete with many illustrations and detailed numerical solutions to prepare the reader to program and calculate evolutionary models</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Stars / Evolution</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Stellar dynamics</subfield></datafield><datafield tag="650" ind1="0" ind2="7"><subfield code="a">Heliumbrennen</subfield><subfield code="0">(DE-588)4778553-6</subfield><subfield code="2">gnd</subfield><subfield code="9">rswk-swf</subfield></datafield><datafield tag="650" ind1="0" ind2="7"><subfield code="a">Sternentwicklung</subfield><subfield code="0">(DE-588)4057365-5</subfield><subfield code="2">gnd</subfield><subfield code="9">rswk-swf</subfield></datafield><datafield tag="650" ind1="0" ind2="7"><subfield code="a">Wasserstoffbrennen</subfield><subfield code="0">(DE-588)4529649-2</subfield><subfield code="2">gnd</subfield><subfield code="9">rswk-swf</subfield></datafield><datafield tag="689" ind1="0" ind2="0"><subfield code="a">Sternentwicklung</subfield><subfield code="0">(DE-588)4057365-5</subfield><subfield code="D">s</subfield></datafield><datafield tag="689" ind1="0" ind2="1"><subfield code="a">Wasserstoffbrennen</subfield><subfield code="0">(DE-588)4529649-2</subfield><subfield code="D">s</subfield></datafield><datafield tag="689" ind1="0" ind2="2"><subfield code="a">Heliumbrennen</subfield><subfield code="0">(DE-588)4778553-6</subfield><subfield code="D">s</subfield></datafield><datafield tag="689" ind1="0" ind2=" "><subfield code="5">DE-604</subfield></datafield><datafield tag="776" ind1="0" ind2="8"><subfield code="i">Erscheint auch als</subfield><subfield code="n">Druckausgabe</subfield><subfield code="z">978-1-107-01656-9</subfield></datafield><datafield tag="856" ind1="4" ind2="0"><subfield code="u">https://doi.org/10.1017/CBO9781139061223</subfield><subfield code="x">Verlag</subfield><subfield code="z">URL des Erstveröffentlichers</subfield><subfield code="3">Volltext</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">ZDB-20-CBO</subfield></datafield><datafield tag="999" ind1=" " ind2=" "><subfield code="a">oai:aleph.bib-bvb.de:BVB01-029354901</subfield></datafield><datafield tag="966" ind1="e" ind2=" "><subfield code="u">https://doi.org/10.1017/CBO9781139061223</subfield><subfield code="l">BSB01</subfield><subfield code="p">ZDB-20-CBO</subfield><subfield code="q">BSB_PDA_CBO</subfield><subfield code="x">Verlag</subfield><subfield code="3">Volltext</subfield></datafield><datafield tag="966" ind1="e" ind2=" "><subfield code="u">https://doi.org/10.1017/CBO9781139061223</subfield><subfield code="l">FHN01</subfield><subfield code="p">ZDB-20-CBO</subfield><subfield code="q">FHN_PDA_CBO</subfield><subfield code="x">Verlag</subfield><subfield code="3">Volltext</subfield></datafield></record></collection> |
| id | DE-604.BV043945930 |
| illustrated | Not Illustrated |
| indexdate | 2024-07-10T07:39:24Z |
| institution | BVB |
| isbn | 9781139061223 |
| language | English |
| oai_aleph_id | oai:aleph.bib-bvb.de:BVB01-029354901 |
| oclc_num | 874382789 |
| open_access_boolean | |
| owner | DE-12 DE-92 |
| owner_facet | DE-12 DE-92 |
| physical | 1 online resource (xvi, 890 pages) |
| psigel | ZDB-20-CBO ZDB-20-CBO BSB_PDA_CBO ZDB-20-CBO FHN_PDA_CBO |
| publishDate | 2013 |
| publishDateSearch | 2013 |
| publishDateSort | 2013 |
| publisher | Cambridge University Press |
| record_format | marc |
| spelling | Iben, Icko 1931- Verfasser aut Stellar evolution physics, Volume 1, Physical processes in stellar interiors Icko Iben Cambridge Cambridge University Press 2013 1 online resource (xvi, 890 pages) txt rdacontent c rdamedia cr rdacarrier Title from publisher's bibliographic system (viewed on 05 Oct 2015) This text describes the microscopic physics operating in stars and demonstrates how stars respond from formation, through hydrogen-burning phases, up to the onset of helium burning. Intended for beginning graduate students and senior undergraduates with a solid background in physics, it illustrates the intricate interplay between the microscopic physical processes and the stars' macroscopic responses. The volume starts with the gravitationally contracting phase which carries the star from formation to the core hydrogen-burning main sequence, through the main sequence phase, through shell hydrogen-burning phases as a red giant, up to the onset of core helium burning. Particular emphasis is placed on describing the gravothermal responses of stars to nuclear transformations in the interior and energy loss from the surface, responses which express the very essence of stellar evolution. The volume is replete with many illustrations and detailed numerical solutions to prepare the reader to program and calculate evolutionary models Stars / Evolution Stellar dynamics Heliumbrennen (DE-588)4778553-6 gnd rswk-swf Sternentwicklung (DE-588)4057365-5 gnd rswk-swf Wasserstoffbrennen (DE-588)4529649-2 gnd rswk-swf Sternentwicklung (DE-588)4057365-5 s Wasserstoffbrennen (DE-588)4529649-2 s Heliumbrennen (DE-588)4778553-6 s DE-604 Erscheint auch als Druckausgabe 978-1-107-01656-9 https://doi.org/10.1017/CBO9781139061223 Verlag URL des Erstveröffentlichers Volltext |
| spellingShingle | Iben, Icko 1931- Stellar evolution physics, Volume 1, Physical processes in stellar interiors Stars / Evolution Stellar dynamics Heliumbrennen (DE-588)4778553-6 gnd Sternentwicklung (DE-588)4057365-5 gnd Wasserstoffbrennen (DE-588)4529649-2 gnd |
| subject_GND | (DE-588)4778553-6 (DE-588)4057365-5 (DE-588)4529649-2 |
| title | Stellar evolution physics, Volume 1, Physical processes in stellar interiors |
| title_auth | Stellar evolution physics, Volume 1, Physical processes in stellar interiors |
| title_exact_search | Stellar evolution physics, Volume 1, Physical processes in stellar interiors |
| title_full | Stellar evolution physics, Volume 1, Physical processes in stellar interiors Icko Iben |
| title_fullStr | Stellar evolution physics, Volume 1, Physical processes in stellar interiors Icko Iben |
| title_full_unstemmed | Stellar evolution physics, Volume 1, Physical processes in stellar interiors Icko Iben |
| title_short | Stellar evolution physics, Volume 1, Physical processes in stellar interiors |
| title_sort | stellar evolution physics volume 1 physical processes in stellar interiors |
| topic | Stars / Evolution Stellar dynamics Heliumbrennen (DE-588)4778553-6 gnd Sternentwicklung (DE-588)4057365-5 gnd Wasserstoffbrennen (DE-588)4529649-2 gnd |
| topic_facet | Stars / Evolution Stellar dynamics Heliumbrennen Sternentwicklung Wasserstoffbrennen |
| url | https://doi.org/10.1017/CBO9781139061223 |
| work_keys_str_mv | AT ibenicko stellarevolutionphysicsvolume1physicalprocessesinstellarinteriors |