The Open Cluster h Per as Seen by Chandra

Details The Open Cluster h Per as Seen by Chandra The Open Cluster h Per as Seen by Chandra

May 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aas...206.3604b&link_type=abstract

American Astronomical Society Meeting 206, #36.04; Bulletin of the American Astronomical Society, Vol. 37, p.488

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Scientific paper

In December, 2004, we observed the open star cluster h Per with Chandra ACIS for 40 ksec. We have identified more than 200 X-ray sources on the image and found optical counterparts for many of them. The ANCHORS pipeline, which we used to process the data, provides homogeneous output products for this and many other star forming regions. Among the outputs are fits to the instrumental low resolution spectra for cool pre-main sequence stars in h Per that yield flux, temperature and absorption for these sources.
Funding for this investigation has been provided by Chandra contract NAS8-39073 and NASA Grant GO5-6007A

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