Accretion of dust grains as a possible origin of metal-poor stars with low α/Fe ratios

Astrophysical Journal

Volumn 598, Issue 1 II, 2003, Pages

  Shigeyama, Toshikazu ^a   Tsujimoto, Takuji ^b  

^a UNIVERSITY OF TOKYO   (Japan)

^b NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN   (Japan)

Author keywords

Galaxies: dwarf; Galaxy: halo; Planetary systems; Stars: abundances; Stars: chemically peculiar

Indexed keywords

EID: 0348156966     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/380479     Document Type: Article

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