X-rays from the star-forming complex W40 Virtual Observatory Resource

Authors
  1. Kuhn M.A.
  2. Getman K.V.
  3. Feigelson E.D.
  4. Reipurth B.
  5. Rodney S.A.,Garmire G.P.
  6. Published by
    CDS
Abstract

The young stellar cluster illuminating the W40 HII region, one of the nearest massive star-forming regions, has been observed with the ACIS detector on board the Chandra X-ray Observatory. Due to its high obscuration, this is a poorly studied stellar cluster with only a handful of bright stars visible in the optical band, including three OB stars identified as primary excitation sources. We detect 225 X-ray sources, of which 85% are confidently identified as young stellar members of the region. Two potential distances of the cluster, 260pc and 600pc, are used in the paper.

Keywords
  1. open-star-clusters
  2. h-ii-regions
  3. x-ray-sources
  4. astronomical-object-identification
  5. infrared-photometry
  6. young-stellar-objects
Bibliographic source Bibcode
2010ApJ...725.2485K
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/725/2485
IVOA Identifier IVOID
ivo://CDS.VizieR/J/ApJ/725/2485
Document Object Identifer DOI
doi:10.26093/cds/vizier.17252485

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History

2012-08-29T13:09:28Z
Resource record created
2012-08-29T13:09:28Z
Created
2018-01-30T07:18:24Z
Updated

Contact

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CDS support team
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