A Parsec-Scale Outflow in the Rosette Molecular Cloud

Details A Parsec-Scale Outflow in the Rosette Molecular Cloud A Parsec-Scale Outflow in the Rosette Molecular Cloud

May 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aas...204.6212p&link_type=abstract

American Astronomical Society Meeting 204, #62.12; Bulletin of the American Astronomical Society, Vol. 36, p.774

Astronomy and Astrophysics

Astronomy

Scientific paper

Ybarra & Phelps (2004) report the discovery of a large angular extent [SII] feature in the Rosette Molecular Cloud (RMC). They suggest that this feature may be a parsec-scale outflow from a young stellar object, possibly associated with an unidentified young stellar object (YSO) in a nearby embedded cluster. Here we report on molecular Hydrogen (H2) observations, obtained with the Lick Observatory 3-meter telescope, that confirm this interpretation. 2MASS data reveal a YSO at the terminus of the [SII] emission, while our H2 data reveal "bulleted" emission, eminating from the YSO and connecting to the optical [SII] emission.

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