Compact Radio and Infrared Sources Near the Centre of the Bipolar Outflow NGC2264D

Details Compact Radio and Infrared Sources Near the Centre of the Bipolar Outflow NGC2264D Compact Radio and Infrared Sources Near the Centre of the Bipolar Outflow NGC2264D

Oct 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990mnras.246..518m&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Vol. 246, NO. 3/OCT1, P. 518, 1990

Astronomy and Astrophysics

Astronomy

12

Scientific paper

A multi-frequency study of the central region of the bipolar outflow NGC 2264D in the Monoceros OB 1 molecular cloud has been made in an attempt to localize and understand its driving source. We have detected a weak (≅0.6 mJy) radio continuum source at 6 cm, using the VLA; a bright (≅270 Jy) H2O maser, using the Haystack Observatory telescope; and near-infrared counterparts to these sources at San Pedro Martir Observatory. Strömgren and JHKL'M photometry of stellar objects in the region was also carried out at this observatory. The star-like object W166, a probable Herbig Be/Ae star, which has strong Ha emission and a near-infrared excess, is located closest to the centroid of the bipolar outflow and is probably its driving source.

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