X-ray emission of YSOs in the Horsehead Nebula

Details X-ray emission of YSOs in the Horsehead Nebula X-ray emission of YSOs in the Horsehead Nebula

Oct 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010xmm..prop...54l&link_type=abstract

XMM-Newton Proposal ID #06712701

Physics

Stars, White Dwarfs, Solar System, Barnard 33

Scientific paper

The Horsehead Nebula is the nearest bright-rimmed cloud to the Sun. In its interior, star formation is taking place at different scales. Deep mid-infrared observations of the forming stars in this region have revealed a large variety of objects, from class I to class III stars, including transitional disk objects. The stars at the limb of the cloud are exposed to the ultraviolet field of sigma Ori, while stars in the interior of the cloud are forming basically in an isolated scenario. By its proximity, the Horsehead Nebula is an excellent laboratory to study the physics of the X-ray emission in young stellar objects at similar evolutionary stages in different environments.

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