Toward understanding the formation of multiple systems * A pilot IRAM-PdBI survey of class 0 objects

Astronomy and Astrophysics

Volumn 512, Issue 6, 2010, Pages

  Maury, A J ^a   André, Ph ^a   Hennebelle, P ^b   Motte, F ^a   Stamatellos, D ^c   Bate, M ^d   Belloche, A ^e   Duchene G ^f,g   Whitworth, A ^c  

^a CEA SACLAY   (France)

^b ECOLE NORMALE SUPÉRIEURE   (France)

^c CARDIFF UNIVERSITY   (United Kingdom)

^d UNIVERSITY OF EXETER   (United Kingdom)

^e MAX PLANCK INSTITUT FÜR RADIOASTRONOMIE   (Germany)

^f UNIVERSITY OF CALIFORNIA   (United States)

^g UNIV GRENOBLE ALPES   (France)

Author keywords

Binaries: general; ISM: clouds; ISM: jets and outflows; Stars: formation

Indexed keywords

CLOUDS;

BINARIES: GENERAL; BINARY FORMATION; BINARY FRACTION; BINARY STAR; CIRCUMSTELLAR; CLASS I; CLASS II; DYNAMICAL EVOLUTION; EVOLUTIONARY STAGE; FORMATION PROCESS; HIGH RESOLUTION; HYDRODYNAMIC MODEL; INFRARED OBSERVATIONS; ISM : CLOUDS; JET AXIS; MASS RATIO; MULTIPLE SYSTEMS; MULTIPLICITY RATE; POSITION ANGLE; PRE-MAIN-SEQUENCE; PROTOSTARS; SECONDARY COMPONENTS; SINGLE COMPONENTS; SMALL SCALE;

STARS;

EID: 77951518369     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200913492     Document Type: Article

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