Chandra Observations of Open Cluster h Per
Abstract
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.
- Publication:
-
Journal of the Royal Astronomical Society of Canada
- Pub Date:
- August 2005
- Bibcode:
- 2005JRASC..99R.136E