Circumstellar Disk Candidates Identified in NGC 2264

Details Circumstellar Disk Candidates Identified in NGC 2264 Circumstellar Disk Candidates Identified in NGC 2264

Dec 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aas...199.8903r&link_type=abstract

American Astronomical Society, 199th AAS Meeting, #89.03; Bulletin of the American Astronomical Society, Vol. 33, p.1435

Astronomy and Astrophysics

Astronomy

Scientific paper

Based on an optical and near-infrared study of a 45′x 45' field in NGC 2264, which includes both S Mon and the Cone Nebula, we identify circumstellar disk candidates using three techniques: excess ultraviolet (U-V) emission, excess near-IR (I-K and H-K) emission, and Hα emission line equivalent widths. We find generally good correlation between disk indicators thought to originate from different physical processes. We find little if any evolution of disk fraction with stellar age or mass.

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