A High Resolution Molecular Line Study of the Bipolar Outflows in the ON2-N Massive Star Forming Region

Details A High Resolution Molecular Line Study of the Bipolar Outflows in the ON2-N Massive Star Forming Region A High Resolution Molecular Line Study of the Bipolar Outflows in the ON2-N Massive Star Forming Region

May 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aas...188.4101s&link_type=abstract

American Astronomical Society, 188th AAS Meeting, #41.01; Bulletin of the American Astronomical Society, Vol. 28, p.885

Astronomy and Astrophysics

Astronomy

Scientific paper

We present high spatial resolution images of the (12) CO(J=1-0), SiO(v=0,J=2-1), H(13) CO(+) (J=1-0) and SO_2(8_{3,5} - 9_{2,8}) emission in the massive star forming region ON2-N. Observations were made with the BIMA mm-wave interferometer. The (12) CO(J=1-0) BIMA data were combined with observations from the NRAO 12m telescope to recover the extended emission in the final images. We find evidence for at least four separate molecular outflows from YSOs within a diameter of 1.5 parsecs. This discovery identifies the area near the ultra compact HII region, G75.78+0.35, as a site of energetic massive star formation.

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