ChandraX-Ray Observations of Young Clusters. I. NGC 2264 Data
Author(s) -
Solange Ramírez,
L. M. Rebull,
J. R. Stauffer,
Thomas Hearty,
Lynne A. Hillenbrand,
B. F. Jones,
Russell B. Makidon,
S. H. Pravdo,
S. E. Strom,
M. W. Werner
Publication year - 2004
Publication title -
the astronomical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.61
H-Index - 271
eISSN - 1538-3881
pISSN - 0004-6256
DOI - 10.1086/383290
Subject(s) - photometry (optics) , physics , astrophysics , stars , light curve , astronomy , infrared , luminosity , variable star , acis , data archive , galaxy , database , computer science
We present results of a Chandra observation of a field in NGC 2264. Theobservations were taken with the ACIS-I camera with an exposure time of 48.1ks. We present a catalog of 263 sources, which includes X-ray luminosity,optical and infrared photometry and X-ray variability information. We found 41variable sources, 14 of which have a flare-like light curve, and 2 of whichhave a pattern of a steady increase or decrease over a 10 hour period. Theoptical and infrared photometry for the stars identified as X-ray sources areconsistent with most of these objects being pre-main sequence stars with agesyounger than 3 Myr.Comment: 36 pages, 13 figures, AJ in press (May 2004
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