The bipolar molecular outflow of V645 Cygni

Details The bipolar molecular outflow of V645 Cygni The bipolar molecular outflow of V645 Cygni

Jun 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...341..288s&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 341, June 1, 1989, p. 288-292.

Astronomy and Astrophysics

Astronomy

14

Interstellar Matter, Line Spectra, Star Formation, Stellar Mass Ejection, Stellar Winds, Variable Stars, Cygnus Constellation, Infrared Astronomy Satellite, Red Shift, Stellar Luminosity, Submillimeter Waves

Scientific paper

A map is presented of the CO J = 3-2 line emission from the cloud associated with V645 Cygni. Line wings extending to 15 km/s on either side of the central velocity can be attributed to a bipolar outflow over a region 1 arcmin in angular extent. The redshifted and blueshifted emission peaks are separated by 20 arcsecs along an axis that is approximately perpendicular to the polarization vector of the visible light. The outflow is of relatively low velocity, low mass, and low mechanical luminosity.

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