Physics
Scientific paper
Sep 2009
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009cfdd.confe.136k&link_type=abstract
Chandra's First Decade of Discovery, Proceedings of the conference held 22-25 September, 2009 in Boston, MA. Edited by Scott Wo
Physics
Stars And Star Formation
Scientific paper
The heavily obscured 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 identified in the optical band, including three OB stars as primary excitation sources. This neglected region deserves detailed investigation. We detect 225 X-ray sources, of which 85% are confidently identified as young stellar members of the region. Our X-ray luminosity function (XLF) analysis confirms the 600 pc distance to W40. Under the assumption of a coeval population with a uniform obscuration the XLF analysis further gives a total stellar population of at least 400 stars down to 0.1Mo. However, we find spatial patches with different source obscurations and Ks-band-excess disk fractions which might suggest that the true underlying population is higher. The location of the strip with highest obscuration is unusual relative to the location of the central cluster and the cold molecular core. The disk fraction has a large variation across the field. Properties of the interesting sources, including diffuse X-ray emission, OB stars, and the young stellar object with a super-hot flare are also discussed.
Feigelson Eric
Garmire Gordon
Getman Konstantin
Kuhn Michael
Reipurth Bo
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