Physics
Scientific paper
Feb 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007ycat..34550903f&link_type=abstract
VizieR On-line Data Catalog: J/A+A/455/903. Originally published in: 2006A&A...455..903F
Physics
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).
Flaccomio Ettore
Micela Giuseppina
Sciortino Salvatore
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