The 300 km s-1 stellar stream near segue 1: Insights from high-resolution spectroscopy of its brightest star

Astrophysical Journal

Volumn 771, Issue 1, 2013, Pages

  Frebel, Anna ^a   Lunnan, Ragnhild ^b   Casey, Andrew R ^a,c   Norris, John E ^c   Wyse, Rosemary F G ^d   Gilmore, Gerard ^e  

^a MASSACHUSETTS INSTITUTE OF TECHNOLOGY   (United States)

^b HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^c AUSTRALIAN NATIONAL UNIVERSITY   (Australia)

^d JOHNS HOPKINS UNIVERSITY   (United States)

^e UNIVERSITY OF CAMBRIDGE   (United Kingdom)

Author keywords

Galaxy: halo; Galaxy: kinematics and dynamics; stars: abundances

Indexed keywords

EID: 84879371112     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1088/0004-637X/771/1/39     Document Type: Article

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