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Stellar evolution physics

Describes how stars respond to microscopic physics, from formation, through hydrogen-burning phases, up to the onset of helium burning.

Detalles Bibliográficos
Autor principal: Iben, Icko
Lenguaje:eng
Publicado: Cambridge University Press 2012
Materias:
Acceso en línea:http://cds.cern.ch/record/1616160
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author Iben, Icko
author_facet Iben, Icko
author_sort Iben, Icko
collection CERN
description Describes how stars respond to microscopic physics, from formation, through hydrogen-burning phases, up to the onset of helium burning.
id cern-1616160
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2012
publisher Cambridge University Press
record_format invenio
spelling cern-16161602021-04-21T22:04:24Zhttp://cds.cern.ch/record/1616160engIben, IckoStellar evolution physicsAstrophysics and AstronomyDescribes how stars respond to microscopic physics, from formation, through hydrogen-burning phases, up to the onset of helium burning.Cambridge University Pressoai:cds.cern.ch:16161602012
spellingShingle Astrophysics and Astronomy
Iben, Icko
Stellar evolution physics
title Stellar evolution physics
title_full Stellar evolution physics
title_fullStr Stellar evolution physics
title_full_unstemmed Stellar evolution physics
title_short Stellar evolution physics
title_sort stellar evolution physics
topic Astrophysics and Astronomy
url http://cds.cern.ch/record/1616160
work_keys_str_mv AT ibenicko stellarevolutionphysics