h and Chi Per: The Loudest Sources?

Details h and Chi Per: The Loudest Sources? h and Chi Per: The Loudest Sources?

Sep 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004cxo..prop.1641e&link_type=abstract

Chandra Proposal ID #06200274

Computer Science

Chandra Proposal Id #06200274

Scientific paper

We propose Chandra observations of the young (14 Myr) stars in the distinctive double cluster h and Chi Per. We have found X-ray sources among the pre-main sequence stars in a ROSAT PSPC image which are more luminous than sources in the younger Orion Nebula cluster. This may imply a higher level of stellar activity than previously measured. High resolution Chandra images will be used to identify the stellar counterparts of X-ray sources, search for a bridge between the clusters, determine the X-ray luminosity distribution, investigate whether the very strong sources are single sources, and study the development of the hot component of the spectra. Optical followup is planned to examine the spectra for emission lines, multiplicity, and rotation.

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