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27 April 2024
 
  » arxiv » astro-ph/0504204

 Article overview



COUP census of X-ray stars in BN-KL and OMC-1S
N. Grosso ; E.D. Feigelson ; K.V. Getman ; L. Townsley ; P. Broos ; E. Flaccomio ; M.J. McCaughrean ; G. Micela ; S. Sciortino ; J. Bally ; N. Smith ; A.A. Muench ; G.P. Garmire ; F. Palla ;
Date 8 Apr 2005
Subject astro-ph
Affiliation4,5), G. Micela , S. Sciortino , J. Bally , N. Smith , A.A. Muench , G.P. Garmire , F. Palla ( Laboratoire d’Astrophysique de Grenoble, Pennsylvania State Univ., Osservatorio Astronomico di Palermo, Univ. of Exeter, AIP, Center for Astroph
AbstractWe present a study of the X-ray sources detected in the vicinity of two density peaks in the Orion Molecular Cloud 1 (OMC-1) behind the Orion Nebula Cluster (ONC), as seen in the exceptionally deep (~10 days) exposure of the Chandra Orion Ultradeep Project (COUP). We focus on a 40"*50" region around the Becklin-Neugebauer object and Kleinmann-Low nebula (collectively BN-KL) and a 60"*75" region around OMC-1S, a secondary star-forming peak some 90" south of BN-KL. Forty-three and sixty X-ray sources were detected in BN-KL and OMC-1S, respectively, of which half and one-third, respectively, were found to be foreground members of the ONC, while the remaining sources are identified as obscured X-ray sources with column densities 22
Source arXiv, astro-ph/0504204
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