Missing low-mass stars in S254-S258 (Mucciarelli+, 2011)

Details Missing low-mass stars in S254-S258 (Mucciarelli+, 2011) Missing low-mass stars in S254-S258 (Mucciarelli+, 2011)

Jun 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011ycat..35339121m&link_type=abstract

VizieR On-line Data Catalog: J/A+A/533/A121. Originally published in: 2011A&A...533A.121M

Computer Science

Stars: Pre-Main Sequence, Ysos, Protostars, X-Ray Sources

Scientific paper

The aim of this study was to find an explanation for the remarkable morphology of the central part of the S254-S258 star forming complex. We performed a deep Chandra X-ray observation of the S254-S258 region in order to efficiently discriminate young stars (with and without circumstellar matter) from the numerous older field stars in the area. We detected 364 X-ray point sources in a 17'x17' field. This X-ray catalog provides, for the first time, a complete sample of all young stars in the region down to about 0.5M&sun;.
(3 data files).

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