A candidate for the exciting source of the powerful molecular outflow NGC 2264G

Details A candidate for the exciting source of the powerful molecular outflow NGC 2264G A candidate for the exciting source of the powerful molecular outflow NGC 2264G

Dec 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989rmxaa..17..115r&link_type=abstract

Revista Mexicana de Astronomia y Astrofisica (ISSN 0185-1101), vol. 17, Dec. 1989, p. 115-119.

Astronomy and Astrophysics

Astronomy

9

Infrared Sources (Astronomy), Molecular Clouds, Nebulae, Pre-Main Sequence Stars, Radio Sources (Astronomy), Ammonia, Star Formation, Stellar Winds

Scientific paper

Continuum observations of the region surrounding the powerful molecular outflow NGC 2264G were made to search for the exciting source of the bipolar molecular outflow in the Monoceros OB1 molecular cloud. In observations made with the VLA at 6-cm and 20-cm, radio continuum was detected. It is proposed that the radio continuum is from the exciting source of the outflow. The spectral index of the source is 0.7 + or - 0.2, consistent with that expected from an ionized stellar wind. The radio continuum source is associated with IRS1, one of the two IR sources proposed as candidates for driving the outflow by Margulis et al. (1989).

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