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astronomy & astrophysics (16) 16
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astrophysics - solar and stellar astrophysics (14) 14
metal-poor stars (9) 9
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abundance (3) 3
astrophysics, cosmology and astronomy (3) 3
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barium stars (3) 3
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cosmology and extragalactic astrophysics (2) 2
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earth and planetary astrophysics (2) 2
element abundance (2) 2
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henize sample (2) 2
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local thermodynamic equilibrium (2) 2
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neutrons (2) 2
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spectroscopic [binaries] (2) 2
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stars: fundamental parameters (2) 2
stellar models (2) 2
technetium (2) 2
temperature (2) 2
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white dwarf stars (2) 2
wind accretion (2) 2
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abundance analysis (1) 1
abundances-stars (1) 1
apm survey (1) 1
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astronomie (1) 1
astronomy (1) 1
astrophysique (1) 1
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Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2015, Volume 446, Issue 3, pp. 2348 - 2362
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2014, Volume 440, Issue 2, pp. 1095 - 1113
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 05/2018, Volume 476, Issue 3, pp. 3086 - 3096
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 2013, Volume 549, pp. A68 - 9
Journal Article
Astronomy & Astrophysics, ISSN 0004-6361, 06/2019, Volume 626, p. A128
Barium (Ba) dwarfs and CH subgiants are the less evolved analogues of Ba and CH giants. They are F- to G-type main-sequence stars polluted with heavy elements... 
Journal Article
Proceedings of the International Astronomical Union, ISSN 1743-9213, 08/2018, Volume 14, Issue S343, pp. 438 - 440
AbstractWe determine Zr and Nb elemental abundances in barium stars to probe the operation temperature of the s-process that occurred in the companion... 
Heavy elements | Barium | Temperature | Neutrons | Abundance | Stellar evolution | Asymptotic giant branch stars | Stellar models | Niobium | Zirconium | Nuclear fusion | Metallicity | Astronomical models | Companion stars
Journal Article
Astronomy & Astrophysics, ISSN 0004-6361, 06/2019, Volume 626, p. A127
Context. Barium and S stars without technetium are red giants and are suspected of being members of binary systems due to their overabundances in heavy... 
Journal Article