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Results 1 - 4 of 4
Stellar laboratories III. New Ba V, Ba VI, and Ba VII oscillator strengths and the barium abundance in the hot white dwarfs G191-B2B and RE0503-289
Volume 9, Issue 17 - article #7
T. Rauch
(1),
K. Werner
(1),
P. Quinet
(2,3),
J. W. Kruk
(4)
((1) Institute for Astronomy and Astrophysics, Eberhard Karls University, Tuebingen, Germany,
(2) Astrophysique et Spectroscopie, Universite de Mons - UMONS, Belgium,
(3) IPNAS, Universite de Liege, Liege, Belgium,
(4) NASA Goddard Space Flight Center, Greenbelt, USA)
arXiv.org - Astrophysics - Volume: 2014, Issue: 25 Apr
arXiv:1404.6094
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Fundamental stellar parameters of three Kepler stars accurately constrained by lithium abundance and rotation
Volume 9, Issue 16 - article #12
K. Liu
,
S. L. Bi
,
T. D. Li
,
Z. J. Tian
and
Z. S. Ge
Astronomy and Astrophysics - Volume: 563, Issue: March 2014
http://dx.doi.org/10.1051/0004-6361/201323277
Abstract
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NASA ADS Abstract Service
Solar Models with Revised Abundance
Volume 6, Issue 23 - article #59
S. L. Bi
,
T. D. Li
,
L. H. Li
and
W. M. Yang
The Astrophysical Journal Letters - Volume: 731, Issue: 2
Abstract
References
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Stellar evolution through the ages: period variations in galactic RRab stars as derived from the GEOS database and TAROT telescopes
Volume 2, Issue 41 - article #11
J.F. Le Borgne
(1 and 2),
A. Paschke
(1 and 3),
J. Vandenbroere
(1),
E. Poretti
(1 and 4),
A. Klotz
(5),
M. Boer
(6),
Y. Damerdji
(6 and 7),
M. Martignoni
(1 and 3),
F. Acerbi
(1)
((1) GEOS
(Groupe Europeen d'Observations Stellaires), France,
(2) Laboratoire d'Astrophysique de Toulouse-Tarbes, Observatoire Midi-Pyrenees, Toulouse, France,
(3) BAV
(Bundesdeutsche Arbeitsgemeinschaft fur Veranderliche Sterne e.V.), Berlin, Germany,
(4) INAF-Osservatorio Astronomico di Brera, Merate, Italy,
(5) Centre d'Etude Spatiale des Rayonnements, Observatoire Midi-Pyrenees, Toulouse, France,
(6) Observatoire de Haute-Provence, France,
(7) Institut d'Astrophysique et de Geophysique de l'Universite de Liege, Liege, Belgium)
arXiv.org - Astrophysics - Volume: 2007, Issue: 11 Oct
arXiv:0710.1846
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