Molecular Hydrogen Emission within the Rosette Molecular Cloud
Abstract
We present near-infrared emission line features from selected regions within the Rosette Molecular Cloud. Spatial relationships between young stellar objects, visible [SII] emission features, and the newly detected near-infrared emission features will be discussed. We acknowledge support from the McNair Scholars Program and the Research Corporation.
- Publication:
-
American Astronomical Society Meeting Abstracts
- Pub Date:
- December 2003
- Bibcode:
- 2003AAS...203.0703Y