Chandra Observations of Open Cluster h Per

Details Chandra Observations of Open Cluster h Per Chandra Observations of Open Cluster h Per

Aug 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005jrasc..99r.136e&link_type=abstract

Journal of the Royal Astronomical Society of Canada, Vol. 99, No. 4, p.136

Astronomy and Astrophysics

Astronomy

Scientific paper

We have obtained a 40 ksec ACIS observation of the open star cluster h Per in December 2004, from which we have identified more than 200 X-ray sources and found optical counterparts for many of them. We are processing the h Per data with the ANCHORS pipeline, which is being used to process Chandra observations of star forming regions in a uniform manner. This will provide fits to the instrumental low-resolution spectra for cool pre-main sequence stars in h Per including fluxes, temperatures, and absorption.

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