A publishing partnership

Chandra X-Ray Observations of Young Clusters. I. NGC 2264 Data

, , , , , , , , , and

© 2004. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation Solange V. Ramírez et al 2004 AJ 127 2659 DOI 10.1086/383290

1538-3881/127/5/2659

Abstract

We present results of a Chandra observation of a field in NGC 2264. The observations were taken with the ACIS-I camera with an exposure time of 48.1 ks. We present a catalog of 263 sources, which includes X-ray luminosity, optical and infrared photometry, and X-ray variability information. We found 41 variable sources, 14 of which have a flarelike light curve, and two of which have a pattern of a steady increase or decrease over a 10 hr period. The optical and infrared photometry for the stars identified as X-ray sources are consistent with most of these objects being pre–main-sequence stars with ages younger than 3 Myr.

Export citation and abstract BibTeX RIS

Please wait… references are loading.
10.1086/383290