Anisotropic mass outflow in Cepheus A

Details Anisotropic mass outflow in Cepheus A Anisotropic mass outflow in Cepheus A

Sep 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...240l.149r&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 240, Sept. 15, 1980, p. L149-L152. Research supported by the Consejo

Astronomy and Astrophysics

Astronomy

153

Cepheid Variables, Interstellar Gas, Molecular Clouds, Radio Sources (Astronomy), Stellar Evolution, Stellar Mass Ejection, Anisotropic Media, B Stars, Carbon Monoxide, Infrared Stars, O Stars

Scientific paper

The detection of high-velocity wings on the CO profile observed toward Cepheus A, a region of star formation in the Cepheus OB3 association, is reported. The velocity extent of the emission is approximately 50 km/s. The blueshifted and redshifted wings have peaks of emission which are spatially separated by approximately 90 arcsec (0.3 pc), suggesting an anisotropic outflow in two opposite directions.

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