X-ray Emission from Young Stars in Suburban Orion

Details X-ray Emission from Young Stars in Suburban Orion X-ray Emission from Young Stars in Suburban Orion

Jan 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004iaus..219..228b&link_type=abstract

Stars as suns : activity, evolution and planets, Proceedings of the 219th symposium of the International Astronomical Union held

Astronomy and Astrophysics

Astronomy

Scientific paper

The Orion Nebula region is the richest site in the sky for study of X-ray emission from pre-main sequence stars harbouring almost a thousand sources in its heart around the O-stars of the Trapezium alone. However not all stars are born within such an environment and the effect of environment on the coronal properties of PMS stars is not well-studied. We present detailed analysis of an XMM-Newton observation of a region on the outskirts of the Orion Nebula 40 arcmin to the north containing over 200 sources and compare coronal properties of this less-dense PMS population to those of the high-density Trapezium cluster.

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