Carbon-enhanced metal-poor stars. III. Main-sequence turnoff stars from the SDSS SEGUE sample

Astrophysical Journal

Volumn 678, Issue 2, 2008, Pages 1351-1371

  Aoki, Wako ^a,b   Beers, Timothy C ^c   Sivarani, Thirupathi ^c   Marsteller, Brian ^c,d   Lee, Young Sun ^c   Honda, Satoshi ^a,e   Norris, John E ^f   Ryan, Sean G ^g   Carollo, Daniela ^f,h  

^a NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN   (Japan)

^b GRADUATE UNIVERSITY FOR ADVANCED STUDIES   (Japan)

^c MICHIGAN STATE UNIVERSITY   (United States)

^d UNIVERSITY OF CALIFORNIA   (United States)

^e Gunma Astronomical Observatory   (Japan)

^f AUSTRALIAN NATIONAL UNIVERSITY   (Australia)

^g UNIVERSITY OF HERTFORDSHIRE   (United Kingdom)

^h OSSERVATORIO ASTRONOMICO DI TORINO   (Italy)

Author keywords

Nuclear reactions, nucleosynthesis, abundances; Stars: abundances; Stars: AGB and post AGB; Stars: Population II

Indexed keywords

EID: 43949096527     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/533517     Document Type: Article

References (83)