PdBI sub-arcsecond study of the SiO microjet in HH212 Origin and collimation of class 0 jets

Astronomy and Astrophysics

Volumn 468, Issue 3, 2007, Pages

  Cabrit, S ^a   Codella, C ^b   Gueth, F ^c   Nisini, B ^d   Gusdorf, A ^e   Dougados, C ^f   Bacciotti, F ^g  

^a OBSERVATOIRE DE PARIS   (France)

^b INAF OSSERVATORIO ASTROFISICO DI TORINO   (Italy)

^c IRAM   (France)

^d INAF OSSERVATORIO ASTRONOMICO DI ROMA   (Italy)

^e DURHAM UNIVERSITY   (United Kingdom)

^f LABORATOIRE D ASTROPHYSIQUE   (France)

^g INAF OSSERVATORIO ASTROFISICO DI ARCETRI   (Italy)

Author keywords

ISM: individual objects: HH212; ISM: jets and outflows; ISM: molecules; Radio lines: ISM; Stars: formation

Indexed keywords

HIGH FREQUENCY TELECOMMUNICATION LINES; INTERFEROMETERS; OPTICAL COLLIMATORS; SILICON COMPOUNDS; STARS; VELOCITY MEASUREMENT;

ISM: JETS AND OUTFLOWS; ISM: MOLECULES; MOLECULAR SYNTHESIS; RADIO LINES: ISM; STARS: FORMATION;

JETS;

EID: 34250737991     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20077387     Document Type: Article

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