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J. E. Ybarra (California State University, Sacramento), R. L. Phelps (California State University, Sacramento; University of California, Davis)
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.
The author(s) of this abstract have provided an email address for comments about the abstract: jybarra@csus.edu
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Bulletin of the American Astronomical Society, 35#5
© 2003. The American Astronomical Soceity.