Star formation in Perseus: Clusters, filaments and the conditions for star formation

Astronomy and Astrophysics

Volumn 440, Issue 1, 2005, Pages 151-161

  Hatchell, J ^a,b   Richer, J S ^c   Fuller, G A ^d   Qualtrough, C J ^c   Ladd, E F ^e   Chandler, C J ^f  

^a MAX PLANCK INSTITUT FÜR RADIOASTRONOMIE   (Germany)

^b UNIVERSITY OF EXETER   (United Kingdom)

^c UNIVERSITY OF CAMBRIDGE   (United Kingdom)

^d UNIVERSITY OF MANCHESTER   (United Kingdom)

^e BUCKNELL UNIVERSITY   (United States)

^f NATIONAL RADIO ASTRONOMY OBSERVATORY   (United States)

Author keywords

Dust, extinction; ISM: clouds; ISM: molecules; ISM: structure; Stars: formation; Submillimeter

Indexed keywords

CLOUDS; CONTINUUM MECHANICS; DUST; GALAXIES; MOLECULES; OPTICAL RESOLVING POWER; PROBABILITY; SURVEYS;

DUST, EXTINCTION; ISM: CLOUD; ISM: MOLECULES; ISM: STRUCTURE; STARS: FORMATION; SUBMILLIMETER;

ASTROPHYSICS;

EID: 24944446033     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20041836     Document Type: Article

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