Progressive star formation in the young SMC cluster NGC 602

Astrophysical Journal

Volumn 665, Issue 2 PART 2, 2007, Pages

  Carlson, Lynn Redding ^a   Sabbi, E ^b   Sirianni, M ^b,j   Hora, J L ^c   Nota, A ^b,j   Meixner, M ^b   Gallagher III, J S ^d   Oey, M S ^e   Pasquali, A ^f   Smith, L J ^g   Tosi, M ^h   Walterbos, R ⁱ  

^a JOHNS HOPKINS UNIVERSITY   (United States)

^b AURA for the European Space Agency   (United States)

^c HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^d UNIVERSITY OF WISCONSIN MADISON   (United States)

^e UNIVERSITY OF MICHIGAN   (United States)

^f MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

^g UNIVERSITY COLLEGE LONDON   (United Kingdom)

^h OSSERVATORIO ASTRONOMICO DI BOLOGNA   (Italy)

ⁱ NEW MEXICO STATE UNIVERSITY   (United States)

^j ESA   (United States)

more..

Author keywords

Galaxies: star clusters; ISM: individual (N90); Magellanic clouds; Open clusters and associations: individual (NGC 602); Stars: formation; stars: pre main sequence

Indexed keywords

EID: 53549123314     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/521023     Document Type: Article

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