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Nature, ISSN 0028-0836, 08/2001, Volume 412, Issue 6849, pp. 793 - 795
About half of the stable nuclei heavier than iron are believed to be synthesized during the late stages of evolution of stars with masses in the range 0.8-8... 
S-PROCESS NUCLEOSYNTHESIS | EVOLUTION | CARBON | BARIUM | CH STARS | NEUTRON-CAPTURE | MULTIDISCIPLINARY SCIENCES | METAL-POOR STAR | AGB STARS | GIANT | Lead | Stars & galaxies | Astronomy
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 1432-0746, 03/2019, Volume 623, p. A151
Context. We previously explored the circumstellar effects on Rb and Zr abundances in a sample (21) of massive Galactic O-rich asymptotic giant branch (AGB)... 
stars: atmospheres | nuclear reactions, nucleosynthesis, abundances | stars: evolution | MHZ SURVEY | RED GIANTS | stars: AGB and post-AGB | S-PROCESS | ASYMPTOTIC GIANT BRANCH | stars: abundances | ATMOSPHERES | EVOLUTION | stars: late-type | STELLAR MODELS | EARLY SOLAR-SYSTEM | PHOTOMETRY | ASTRONOMY & ASTROPHYSICS | VARIABLES | Physics | Astrophysics
Journal Article
Astronomy & Astrophysics, ISSN 0004-6361, 06/2012, Volume 542, pp. 1 - 1
The relatively wide spread in the derived metallicities Fe/H of M dwarfs shows that various approaches have not yet converged to consistency. The presence of... 
Band spectra | Spectroscopy | Infrared | Metallicity | Consistency | Spectroscopic analysis | Spectra | Astronomy
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 2009, Volume 508, Issue 2, pp. 909 - 922
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 04/2018, Volume 612, p. A65
Context. Extremely metal-poor (EMP) stars provide us with indirect information on the first generations of massive stars. The TOPoS survey has been designed to... 
Galaxy: halo | Stars: abundances | Stars: population II | Galaxy: formation | Cosmology: observations | Galaxy: abundances
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 2013, Volume 560, pp. A15 - np
Journal Article