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Astronomy and Astrophysics, ISSN 0004-6361, 11/2016, Volume 595, p. A60
Journal Article
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 03/2016, Volume 587, p. A30
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 02/2011, Volume 526, Issue 9, p. A69
The HERMES high-resolution spectrograph project aims at exploiting the specific potential of small but flexible telescopes in observational astrophysics. The... 
instrumentation: spectrographs | techniques: radial velocities | stars: abundances | techniques: spectroscopic | ESO | SIGNATURES | ASTRONOMY & ASTROPHYSICS | BINARIES | SPECTRA | Physics - Instrumentation and Methods for Astrophysics
Journal Article
Nature, ISSN 0028-0836, 01/2015, Volume 517, Issue 7533, pp. 174 - 176
Roughly half of the heavy elements (atomic mass greater than that of iron) are believed to be synthesized in the late evolutionary stages of stars with masses... 
DREDGE-UP | TECHNETIUM | EVOLUTION | NIOBIUM ABUNDANCES | MODELS | MULTIDISCIPLINARY SCIENCES | CHEMICAL-COMPOSITION | S-PROCESS | NUCLEOSYNTHESIS | ASYMPTOTIC GIANT BRANCH | AGB STARS | Stellar evolution | Chemical properties | Observations | Heavy elements (Cosmochemistry) | Properties | Stars | Neutrons | Temperature | Ratios | Stars & galaxies | Methods | Physics - Solar and Stellar Astrophysics | Physics | Astrophysics
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
Astronomy and Astrophysics, ISSN 0004-6361, 2011, Volume 532, p. A13
Aims. Surface brightness asymmetries are a very common feature of stars. Among other effects they cause a difference between the projected barycentre and... 
convection | methods: analytical | parallaxes | space vehicles | supergiants | astrometry | ASTRONOMY & ASTROPHYSICS | BETELGEUSE | SIMULATIONS | ATMOSPHERE
Journal Article