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α-, r-, and s-process element trends in the Galactic thin and thick disks

Author
BENSBY, T1 2 ; FELTZING, S1 ; LUNDSTRÖM, I1 ; ILYIN, I3
[1] Lund Observatory, Box 43, 221 00 Lund, Sweden
[2] Department of Astronomy, 921 Dennison Building, University of Michigan, Ann Arbor, MI 48109-1090, United States
[3] Astrophysical Institute Potsdam, An der Sternwarte 16, 14482 Potsdam, Germany
Source

Astronomy and astrophysics (Berlin. Print). 2005, Vol 433, Num 1, pp 185-203, 19 p ; ref : 72 ref

CODEN
AAEJAF
ISSN
0004-6361
Scientific domain
Astronomy earth cosmic environment
Publisher
EDP Sciences, Les Ulis
Publication country
France
Document type
Article
Language
English
Author keyword
Galaxy: abundances -Galaxy: kinematics and dynamics Galaxy: disk Galaxy: formation stars: abundances stars: fundamental parameters
Keyword (fr)
Abondance stellaire Abondance élément Cinématique stellaire Disque galactique Dynamique Etoile G Etoile naine Formation galaxies Galaxies disques Invariant Paramètre physique Plan galactique Processus r Processus s Rapport signal bruit Voisinage solaire
Keyword (en)
Stellar abundance Element abundance Stellar kinematics Galactic disks Dynamics G stars Dwarf stars Galaxy formation Disk galaxies Invariant Physical parameter Galactic planes r process s process Signal-to-noise ratio Solar neighborhood
Keyword (es)
Abundancia estelar Cinematica estelar Invariante Parámetro físico Vecindad solar
Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
16592745

Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS

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