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, University of Notre Dame
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Results 1 - 4 of 4
Lithium abundances of halo dwarfs based on excitation temperatures. II. NLTE
Volume 5, Issue 15 - article #10
A. Hosford
,
A.E. Garcia Perez
,
R. Collet
,
S.G. Ryan
,
J.E. Norris
,
K.A. Olive
arXiv.org - Astrophysics - Volume: 2010, Issue: 9 Apr
arXiv:1004.0863
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pdf
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ps
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other
]
6Li/7Li estimates for metal-poor stars
Volume 4, Issue 40 - article #1
A.E. Garcia Perez
,
W. Aoki
,
S. Inoue
,
S.G. Ryan
,
T.K. Suzuki
,
M. Chiba
arXiv.org - Astrophysics - Volume: 2009, Issue: 2 Oct
arXiv:0909.5163
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ps
,
pdf
,
other
]
Lithium abundances of halo dwarfs based on excitation temperature. I. LTE
Volume 3, Issue 47 - article #11
A. Hosford
,
S.G. Ryan
,
A.E. Garcia Perez
,
J.E. Norris
,
K.A. Olive
arXiv.org - Astrophysics - Volume: 2008, Issue: 20 Nov
arXiv:0811.2506
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ps
,
pdf
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other
]
Experimental Mg I oscillator strengths and radiative lifetimes for astrophysical applications on metal-poor stars - New data for the Mg I b triplet
Volume 1, Issue 36 - article #4
M. Aldenius
(1),
J.D. Tanner
(2),
S. Johansson
(1),
H. Lundberg
(3),
S.G. Ryan
(2 and 4)
((1) Lund Observatory,
(2) The Open University,
(3) Lund Institute of Technology,
(4) University of Hertfordshire)
ArXiv - Astrophysics
astro-ph/0610033 [
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Results 1 - 4 of 4
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