Catching the Third Generation of Ysos in the CEPB/S155 Interface Region

Details Catching the Third Generation of Ysos in the CEPB/S155 Interface Region Catching the Third Generation of Ysos in the CEPB/S155 Interface Region

Sep 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002cxo..prop.1071g&link_type=abstract

Chandra Proposal ID #04200052

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Chandra Proposal Id #04200052

Scientific paper

In a single Chandra field we will make a snapshot of the violent interaction of young stars with their natal cloud. We will be able to study the properties of two generation of young stars, one, already emerged from the cloud, and another, deeply embedded into it. The second includes the nearest known candidate of high mass protostellar object (HMPO). Our goals are: to confirm the YSO status of IR sources, compare the spectra and variability for different types of YSOs, search for the extended emission from O-star winds, construct X-ray luminosity and initial mass functions of the emerged generation, become acquainted with the X-ray properties of HMPO; and study the star formation history of this region.

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