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...
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Format: | Elektronisch E-Book |
Sprache: | English |
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Cambridge
Cambridge University Press
2013
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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 |
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Datensatz im Suchindex
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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 |
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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 |
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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 |