Molecular Hydrogen Emission within the Rosette Molecular Cloud

Astronomy and Astrophysics – Astronomy

Scientific paper

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Scientific paper

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.

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