A Subarcsecond Radio Binary Associated with AFGL 4029

Details A Subarcsecond Radio Binary Associated with AFGL 4029 A Subarcsecond Radio Binary Associated with AFGL 4029

Jan 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003rmxac..15..209z&link_type=abstract

Winds, Bubbles, and Explosions: a conference to honor John Dyson, Pátzcuaro, Michoacán, México, September 9-13, 2002 (Eds. S. J.

Astronomy and Astrophysics

Astronomy

Individual:(Afgl 4029), Ism: H Ii Regions, Ism: Jets And Outflows, Radio Continuum: Stars: Formation

Scientific paper

We present sensitive, high angular resolution (0''.3) Very Large Array observations made at 3.6 cm of the bright infrared source AFGL 4029. We find that the radio source G 138.295+1.555, associated with AFGL 4029-IRS1, is actually a subarcsecod binary. There is also fainter emission extending in the east-west direction and emanating from G 138.295+1.555(S), the southern component of the binary. We then identify G 138.295+1.555(S) as the exciting source of the optical and molecular outflow observed in this region.

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