X-ray emission in Orion Nebula young stars (Flaccomio+, 2005)

Details X-ray emission in Orion Nebula young stars (Flaccomio+, 2005) X-ray emission in Orion Nebula young stars (Flaccomio+, 2005)

Jul 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006ycat..21600450f&link_type=abstract

VizieR On-line Data Catalog: J/ApJS/160/450. Originally published in: 2005ApJS..160..450F

Physics

X-Ray Sources, Clusters: Open, Stars: Pre-Main Sequence, Equivalent Widths

Scientific paper

We investigate the spatial distribution of X-ray-emitting plasma in a sample of young Orion Nebula Cluster stars by modulation of their X-ray light curves due to stellar rotation. The study, part of the Chandra Orion Ultradeep Project (COUP, Cat. ), is made possible by the exceptional length of the observation: 10 days of ACIS integration during a time span of 13 days, yielding a total of 1616 detected sources in the 17'x17' field of view. We here focus on a subsample of 233 X-ray-bright stars with known rotational periods. We search for X-ray modulation using the Lomb Normalized Periodogram method.
(1 data file).

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