Models for extremely metal-poor halo stars

Astronomy and Astrophysics

Volumn 422, Issue 1, 2004, Pages 217-223

  Weiss, A ^a   Schlattl, H ^a,b   Salaris, M ^b   Cassisi, S ^c  

^a MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^b LIVERPOOL JOHN MOORES UNIVERSITY   (United Kingdom)

^c INAF OSSERVATORIO ASTRONOMICO DI COLLURANIA   (Italy)

Author keywords

Stars: Abundances; Stars: Evolution stars: Individual: He 0107 5240; Stars: Interiors; Stars: Low mass, brown dwarfs

Indexed keywords

ASTROPHYSICS; COMPOSITION; GALAXIES; NITROGEN; OXYGEN; PROTONS;

STARS:ABUNDANCES; STARS:EVOLOTION; STARS:INDIVIDUAL:HE 0107-5240; STARS:INTERIORS; STARS:LOW MASS, BROWN DWARFS;

ATMOSPHERIC THERMODYNAMICS;

EID: 3142751900     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20040248     Document Type: Article

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