The spatial distribution of star formation in the solar neighbourhood: Do all stars form in dense clusters?

Monthly Notices of the Royal Astronomical Society: Letters

Volumn 409, Issue 1, 2010, Pages

  Bressert, E ^a,b   Bastian, N ^a,c   Gutermuth, R ^d   Megeath, S T ^e   Allen, L ^f   Evans, Neal J ^g   Rebull, L M ^h   Hatchell, J ^a   Johnstone, D ^i,j   Bourke, T L ^b   Cieza, L A ^k   Harvey, P M ^g   Merin, B ^l   Ray, T P ^m   Tothill, N F H ^a,n  

^a UNIVERSITY OF EXETER   (United Kingdom)

^b HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^c UNIVERSITY OF CAMBRIDGE   (United Kingdom)

^d UNIVERSITY OF MASSACHUSETTS   (United States)

^e UNIVERSITY OF TOLEDO   (United States)

^f NATIONAL OPTICAL ASTRONOMY OBSERVATORY   (United States)

^g UNIVERSITY OF TEXAS AT AUSTIN   (United States)

^h CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

ⁱ NATIONAL RESEARCH COUNCIL CANADA   (Canada)

^j UNIVERSITY OF VICTORIA   (Canada)

^k UNIVERSITY OF HAWAII   (United States)

^l EUROPEAN SPACE AGENCY   (France)

^m DUBLIN INSTITUTE FOR ADVANCED STUDIES   (Ireland)

ⁿ UNIVERSITY OF NEW SOUTH WALES   (Australia)

more..

Author keywords

Infrared: stars; Open clusters and associations: general; Stars: formation; Stars: protostars

Indexed keywords

EID: 79952469457     PISSN: 17453933     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1745-3933.2010.00946.x     Document Type: Letter

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