Two distinct ancient components in the sculptor dwarf spheroidal galaxy: First results from the dwarf abundances and radial velocities team

Astrophysical Journal

Volumn 617, Issue 2 II, 2004, Pages

  Tolstoy, Eline ^a   Irwin, M J ^b   Helmi, A ^a   Battaglia, G ^a   Jablonka, P ^c   Hill, V ^c   Venn, K A ^d   Shetrone, M D ^e   Letarte, B ^a   Cole, A A ^a   Primas, F ^f   Francois, P ^c   Arimoto, N ^g   Sadakane, K ^h   Kaufer, A ⁱ   Szeifert, T ⁱ   Abel, T ^j  

^a UNIVERSITY OF GRONINGEN   (Netherlands)

^b UNIVERSITY OF CAMBRIDGE   (United Kingdom)

^c OBSERVATOIRE DE PARIS   (France)

^d MACALESTER COLLEGE   (United States)

^e The University of Texas at Austin   (United States)

^f EUROPEAN SOUTHERN OBSERVATORY   (Germany)

^g NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN   (Japan)

^h OSAKA KYOIKU UNIVERSITY   (Japan)

ⁱ EUROPEAN SOUTHERN OBSERVATORY   (Chile)

^j PENNSYLVANIA STATE UNIVERSITY   (United States)

more..

Author keywords

Galaxies: abundances; Galaxies: evolution; Galaxies: individual (Sculptor); Galaxies: kinematics and dynamics

Indexed keywords

EID: 13944255147     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/427388     Document Type: Article

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