ACIS-I observations of NGC 2264 (Flaccomio+, 2006)

Physics

Scientific paper

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Clusters: Open, Stars: Pre-Main Sequence, X-Ray Sources, Photometry: Infrared

Scientific paper

This paper's goal is to improve the member census of the NGC 2264 star-forming region and study the origin of X-ray activity in young PMS stars. We analyze a deep, 100ks long, Chandra ACIS observation covering a 17'x17' field in NGC 2264. The preferential detection in X-rays of low-mass PMS stars gives strong indications of their membership. We study X-ray activity as a function of stellar and circumstellar characteristics by correlating the X-ray luminosities, temperatures, and absorptions with optical and near-infrared data from the literature.
(4 data files).

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