A multi-wavelength study of a double intermediate-mass protostar - From large-scale structure to collimated jets

Astronomy and Astrophysics

Volumn 493, Issue 2, 2009, Pages 547-556

  Forbrich, J ^a,b,c   Stanke, Th ^d,e   Klein, R ^f,g   Henning, Th ^h   Menten, K M ^a   Schreyer, K ^b   Posselt, B ^b,c,f  

^a MAX PLANCK INSTITUT FÜR RADIOASTRONOMIE   (Germany)

^b Astrophysikalisches Institut   (Germany)

^c HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^d UNIVERSITY OF HAWAII   (United States)

^e EUROPEAN SOUTHERN OBSERVATORY   (Germany)

^f MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

^g UNIVERSITY OF CALIFORNIA   (United States)

^h MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

Author keywords

ISM: jets and outflows; Stars: formation

Indexed keywords

JETS; LUMINANCE; MOLECULAR MASS;

ACCRETION RATES; CHEMICAL COMPOSITIONS; CIRCUMSTELLAR; COLLIMATED JETS; COLUMN DENSITIES; CONTINUUM SOURCES; DRIVING SOURCES; EVOLUTIONARY STAGES; FAR-INFRARED; GAS MASS; HIGH-MASS STARS; INDIVIDUAL COMPONENTS; ISM: JETS AND OUTFLOWS; LARGE-SCALE STRUCTURES; LINEAR SEPARATIONS; MASS STARS; MOLECULAR OUTFLOWS; MULTI WAVELENGTHS; MULTI-WAVELENGTH STUDIES; NEAR INFRA REDS; PROTOSTAR; PROTOSTELLAR OBJECTS; RADIO CONTINUUMS; SPITZER; STARS: FORMATION; SUB MILLIMETERS; TIME-SCALE; TWO COMPONENTS; TWO SOURCES; WAVELENGTH RANGES;

STARS;

EID: 59049084877     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:200810598     Document Type: Article

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