ASCA Observation of the Young Stellar Cluster, IC348

Details ASCA Observation of the Young Stellar Cluster, IC348 ASCA Observation of the Young Stellar Cluster, IC348

Dec 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999sf99.proc..316n&link_type=abstract

Star Formation 1999, Proceedings of Star Formation 1999, held in Nagoya, Japan, June 21 - 25, 1999, Editor: T. Nakamoto, Nobeyam

Computer Science

Scientific paper

We observed the young stellar cluster IC348 located in the Perceus molecular cloud complex with ASCA in the 0.5-10 keV band. X-ray emission was detected from eleven sources, which were all identified with the ROSAT X-ray sources. Temperatures of these sources were in the range of 1.5-3.9 keV, whereas the ROSAT results showed somewhat lower temperature of ~ 1 keV on average. We also derived the integrated spectrum in the IC348 center region within 4' radius. The spectrum was fit to a two-temperature thin thermal model, which give a better fit than a single temperature model. Present results suggest that the X-ray emission from the core region of IC348 comes from multi-temperature plasmas.

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