Stellar evolution physics, Volume 2, Advanced evolution of single stars:
This volume explains the microscopic physics operating in stars in advanced stages of their evolution and describes with many numerical examples and illustrations how they respond to this microphysics. Models of low and intermediate mass are evolved through the core helium-burning phase, the asympto...
Saved in:
| Main Author: | |
|---|---|
| Format: | Electronic eBook |
| Language: | English |
| Published: |
Cambridge
Cambridge University Press
2013
|
| Subjects: | |
| Online Access: | BSB01 FHN01 Volltext |
| Summary: | This volume explains the microscopic physics operating in stars in advanced stages of their evolution and describes with many numerical examples and illustrations how they respond to this microphysics. Models of low and intermediate mass are evolved through the core helium-burning phase, the asymptotic giant branch phase (alternating shell hydrogen and helium burning) and through the final cooling white dwarf phase. A massive model is carried from the core helium-burning phase through core and shell carbon-burning phases. Gravothermal responses to nuclear reaction-induced transformations and energy loss from the surface are described in detail. Written for senior graduate students and researchers who have mastered the principles of stellar evolution, as developed in the first volume of Stellar Evolution Physics, sufficient attention is paid to how numerical solutions are obtained to enable the reader to engage in model construction on a professional level |
| Item Description: | Title from publisher's bibliographic system (viewed on 05 Oct 2015) |
| Physical Description: | 1 online resource (x, pages 893-1495) |
| ISBN: | 9781139061230 |
| DOI: | 10.1017/CBO9781139061230 |
Staff View
MARC
| LEADER | 00000nmm a2200000zc 4500 | ||
|---|---|---|---|
| 001 | BV043945936 | ||
| 003 | DE-604 | ||
| 005 | 00000000000000.0 | ||
| 007 | cr|uuu---uuuuu | ||
| 008 | 161206s2013 |||| o||u| ||||||eng d | ||
| 020 | |a 9781139061230 |c Online |9 978-1-139-06123-0 | ||
| 024 | 7 | |a 10.1017/CBO9781139061230 |2 doi | |
| 035 | |a (ZDB-20-CBO)CR9781139061230 | ||
| 035 | |a (OCoLC)874382790 | ||
| 035 | |a (DE-599)BVBBV043945936 | ||
| 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 2, Advanced evolution of single stars |c Icko Iben |
| 264 | 1 | |a Cambridge |b Cambridge University Press |c 2013 | |
| 300 | |a 1 online resource (x, pages 893-1495) | ||
| 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 volume explains the microscopic physics operating in stars in advanced stages of their evolution and describes with many numerical examples and illustrations how they respond to this microphysics. Models of low and intermediate mass are evolved through the core helium-burning phase, the asymptotic giant branch phase (alternating shell hydrogen and helium burning) and through the final cooling white dwarf phase. A massive model is carried from the core helium-burning phase through core and shell carbon-burning phases. Gravothermal responses to nuclear reaction-induced transformations and energy loss from the surface are described in detail. Written for senior graduate students and researchers who have mastered the principles of stellar evolution, as developed in the first volume of Stellar Evolution Physics, sufficient attention is paid to how numerical solutions are obtained to enable the reader to engage in model construction on a professional level | ||
| 650 | 4 | |a Stars / Evolution | |
| 650 | 4 | |a Stellar dynamics | |
| 776 | 0 | 8 | |i Erscheint auch als |n Druckausgabe |z 978-1-107-01657-6 |
| 856 | 4 | 0 | |u https://doi.org/10.1017/CBO9781139061230 |x Verlag |z URL des Erstveröffentlichers |3 Volltext |
| 912 | |a ZDB-20-CBO | ||
| 999 | |a oai:aleph.bib-bvb.de:BVB01-029354907 | ||
| 966 | e | |u https://doi.org/10.1017/CBO9781139061230 |l BSB01 |p ZDB-20-CBO |q BSB_PDA_CBO |x Verlag |3 Volltext | |
| 966 | e | |u https://doi.org/10.1017/CBO9781139061230 |l FHN01 |p ZDB-20-CBO |q FHN_PDA_CBO |x Verlag |3 Volltext | |
Record in the Search Index
| _version_ | 1804176892645867520 |
|---|---|
| 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 | BV043945936 |
| collection | ZDB-20-CBO |
| ctrlnum | (ZDB-20-CBO)CR9781139061230 (OCoLC)874382790 (DE-599)BVBBV043945936 |
| 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/CBO9781139061230 |
| format | Electronic eBook |
| fullrecord | <?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>02466nmm a2200397zc 4500</leader><controlfield tag="001">BV043945936</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">9781139061230</subfield><subfield code="c">Online</subfield><subfield code="9">978-1-139-06123-0</subfield></datafield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1017/CBO9781139061230</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(ZDB-20-CBO)CR9781139061230</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(OCoLC)874382790</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-599)BVBBV043945936</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 2, Advanced evolution of single stars</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 (x, pages 893-1495)</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 volume explains the microscopic physics operating in stars in advanced stages of their evolution and describes with many numerical examples and illustrations how they respond to this microphysics. Models of low and intermediate mass are evolved through the core helium-burning phase, the asymptotic giant branch phase (alternating shell hydrogen and helium burning) and through the final cooling white dwarf phase. A massive model is carried from the core helium-burning phase through core and shell carbon-burning phases. Gravothermal responses to nuclear reaction-induced transformations and energy loss from the surface are described in detail. Written for senior graduate students and researchers who have mastered the principles of stellar evolution, as developed in the first volume of Stellar Evolution Physics, sufficient attention is paid to how numerical solutions are obtained to enable the reader to engage in model construction on a professional level</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="776" ind1="0" ind2="8"><subfield code="i">Erscheint auch als</subfield><subfield code="n">Druckausgabe</subfield><subfield code="z">978-1-107-01657-6</subfield></datafield><datafield tag="856" ind1="4" ind2="0"><subfield code="u">https://doi.org/10.1017/CBO9781139061230</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:BVB01-029354907</subfield></datafield><datafield tag="966" ind1="e" ind2=" "><subfield code="u">https://doi.org/10.1017/CBO9781139061230</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/CBO9781139061230</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.BV043945936 |
| illustrated | Not Illustrated |
| indexdate | 2024-07-10T07:39:24Z |
| institution | BVB |
| isbn | 9781139061230 |
| language | English |
| oai_aleph_id | oai:aleph.bib-bvb.de:BVB01-029354907 |
| oclc_num | 874382790 |
| open_access_boolean | |
| owner | DE-12 DE-92 |
| owner_facet | DE-12 DE-92 |
| physical | 1 online resource (x, pages 893-1495) |
| 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 2, Advanced evolution of single stars Icko Iben Cambridge Cambridge University Press 2013 1 online resource (x, pages 893-1495) txt rdacontent c rdamedia cr rdacarrier Title from publisher's bibliographic system (viewed on 05 Oct 2015) This volume explains the microscopic physics operating in stars in advanced stages of their evolution and describes with many numerical examples and illustrations how they respond to this microphysics. Models of low and intermediate mass are evolved through the core helium-burning phase, the asymptotic giant branch phase (alternating shell hydrogen and helium burning) and through the final cooling white dwarf phase. A massive model is carried from the core helium-burning phase through core and shell carbon-burning phases. Gravothermal responses to nuclear reaction-induced transformations and energy loss from the surface are described in detail. Written for senior graduate students and researchers who have mastered the principles of stellar evolution, as developed in the first volume of Stellar Evolution Physics, sufficient attention is paid to how numerical solutions are obtained to enable the reader to engage in model construction on a professional level Stars / Evolution Stellar dynamics Erscheint auch als Druckausgabe 978-1-107-01657-6 https://doi.org/10.1017/CBO9781139061230 Verlag URL des Erstveröffentlichers Volltext |
| spellingShingle | Iben, Icko 1931- Stellar evolution physics, Volume 2, Advanced evolution of single stars Stars / Evolution Stellar dynamics |
| title | Stellar evolution physics, Volume 2, Advanced evolution of single stars |
| title_auth | Stellar evolution physics, Volume 2, Advanced evolution of single stars |
| title_exact_search | Stellar evolution physics, Volume 2, Advanced evolution of single stars |
| title_full | Stellar evolution physics, Volume 2, Advanced evolution of single stars Icko Iben |
| title_fullStr | Stellar evolution physics, Volume 2, Advanced evolution of single stars Icko Iben |
| title_full_unstemmed | Stellar evolution physics, Volume 2, Advanced evolution of single stars Icko Iben |
| title_short | Stellar evolution physics, Volume 2, Advanced evolution of single stars |
| title_sort | stellar evolution physics volume 2 advanced evolution of single stars |
| topic | Stars / Evolution Stellar dynamics |
| topic_facet | Stars / Evolution Stellar dynamics |
| url | https://doi.org/10.1017/CBO9781139061230 |
| work_keys_str_mv | AT ibenicko stellarevolutionphysicsvolume2advancedevolutionofsinglestars |