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Results 1 - 4 of 4
Fates of the oldest intermediate-mass stars - Primordial to Extremely Metal-Poor AGB and Super-AGB Stars: White Dwarf or Supernova progenitors. (arXiv:1810.00982v1 [astro-ph.SR])
Volume 13, Issue 40 - article #2
Pilar Gil-Pons
,
Carolyn L. Doherty
,
Jordi L. Gutiérrez
,
Lionel Siess
,
Simon W. Campbell
,
Herbert B. Lau
,
John C. Lattanzio
http://arxiv.org/abs/1810.00982
Super and massive AGB stars - III. Nucleosynthesis in metal-poor and very metal-poor stars - Z=0.001 and 0.0001
Volume 9, Issue 12 - article #7
Carolyn L. Doherty
,
Pilar Gil-Pons
,
Herbert H.B. Lau
,
John C. Lattanzio
,
Lionel Siess
,
Simon W. Campbell
arXiv.org - Astrophysics - Volume: 2014, Issue: 21 Mar
arXiv:1403.5054
[
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ps
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]
Super and massive AGB stars – II. Nucleosynthesis and yields –
Z
= 0.02, 0.008 and 0.004
Volume 9, Issue 4 - article #36
Carolyn L. Doherty
,
Pilar Gil-Pons
,
Herbert H. B Lau
,
John C. Lattanzio
,
and
Lionel Siess
Monthly Notices of the Royal Astronomical Society - Volume: 437, Issue: 1
Abstract
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The late stages of the evolution of intermediate-mass primordial stars: the effects of overshooting
Volume 1, Issue 46 - article #5
Pilar Gil-Pons
,
Jordi Gutierrez
,
Enrique Garcia-Berro
ArXiv - Astrophysics
astro-ph/0612267 [
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Results 1 - 4 of 4
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