High-velocity molecular jets and bullets from IRAS 03282 + 3035

Details High-velocity molecular jets and bullets from IRAS 03282 + 3035 High-velocity molecular jets and bullets from IRAS 03282 + 3035

Nov 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26a...251..639b&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 251, no. 2, Nov. 1991, p. 639-648. Research supported by CICYT.

Astronomy and Astrophysics

Astronomy

72

Jet Flow, Molecular Clouds, Molecular Flow, Star Formation, Carbon Monoxide, Infrared Astronomy Satellite, Interstellar Gas, Luminosity, Stellar Mass

Scientific paper

A new key to the understanding of the physical structure and origin of bipolar outflows has been provided by the detection of high-velocity molecular bullets in three flows: L1448, HH 7-11, and Rho Oph A. This paper reports the detection of this kind of bullet in the IRAS 3282 outflow. The observations seem to confirm that, in many bipolar outflows, an important part of the mass loss occurs in the form of sporadic ejection of neutral matter.

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