Virtual Journal of Nuclear Astrophysics
Edited by
Honey Arora
, Michigan State University and
Fry Fang
, University of Notre Dame
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Results 1 - 5 of 5
Be and Bn stars: Balmer discontinuity and stellar-class relationship★
Virtual Journal - Volume 18, Issue 5 - article #15
Y. R. Cochetti
,
J. Zorec
,
L. S. Cidale
,
M. L. Arias
,
Y. Aidelman
,
A. F. Torres
,
Y. Frémat
,
A. Granada
Astronomy & Astrophysics
http://feedproxy.google.com/~r/edp_aa/~3/t9_ie8ZlHLM/201936444
Populations of rotating stars - III. SYCLIST, the new Geneva population synthesis code
Virtual Journal - Volume 12, Issue 21 - article #110
C. Georgy
,
A. Granada
,
S. Ekström
,
G. Meynet
,
R. I. Anderson
,
A. Wyttenbach
,
P. Eggenberger
and
A. Maeder
Astronomy and Astrophysics - Volume: 566, Issue: June 2014
http://dx.doi.org/10.1051/0004-6361/201423881
Abstract
Full HTML
PDF (2.053 MB)
ePUB (2.246 MB)
References
NASA ADS Abstract Service
Grids of stellar models with rotation - III. Models from 0.8 to 120 M
⊙
at a metallicity Z = 0.002
Virtual Journal - Volume 11, Issue 45 - article #28
C. Georgy
,
S. Ekström
,
P. Eggenberger
,
G. Meynet
,
L. Haemmerlé
,
A. Maeder
,
A. Granada
,
J. H. Groh
,
R. Hirschi
,
N. Mowlavi
,
et al.
(4 more)
N. Yusof
,
C. Charbonnel
,
T. Decressin
and
F. Barblan
Astronomy and Astrophysics - Volume: 558, Issue: October 2013
http://dx.doi.org/10.1051/0004-6361/201322178
Abstract
Full HTML
PDF (789.9 KB)
References
Tables at CDS
NASA ADS Abstract Service
Populations of rotating stars - I. Models from 1.7 to 15 M
⊙
at Z = 0.014, 0.006, and 0.002 with Ω/Ω
crit
between 0 and 1
Virtual Journal - Volume 11, Issue 23 - article #18
C. Georgy
,
S. Ekström
,
A. Granada
,
G. Meynet
,
N. Mowlavi
,
P. Eggenberger
and
A. Maeder
Astronomy and Astrophysics - Volume: 553, Issue: May 2013
http://dx.doi.org/10.1051/0004-6361/201220558
Abstract
Full HTML
PDF (3.782 MB)
References
Online Material
Tables at CDS
NASA ADS Abstract Service
s-Process in Low Metallicity Stars. I. Theoretical Predictions
Virtual Journal - Volume 8, Issue 6 - article #6
S. Bisterzo
(1),
R. Gallino
(1),
O. Straniero
(2),
S. Cristallo
(2 and 3),
F. Kaeppeler
(4)
((1) Dipartimento di Fisica Generale, Universita' di Torino, Via P. Giuria 1, Torino, Italy,
(2) INAF Osservatorio Astronomico di Collurania, via M. Maggini, Teramo, Italy,
(3) Departamento de Fisica Teorica y del Cosmos, Universidad de Granada, Campus de Fuentenueva, Granada, Spain,
(4) Karlsruhe Institute of Technology, Campus Nord, Forschungszentrum Karlsruhe, Institut fur Kernphysik, Karlsruhe, Germany)
arXiv.org - Astrophysics - Volume: 2010, Issue: 5 Feb
arXiv:1001.5376
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