Large-scale young Gould Belt stars across Orion

(2) European Southern Observatory (ESO) - Chile; (3) INAF - Catania Astrophysical Observatory; (4) Observatoire Astronomique de Strasbourg; A. Frasca (3); CNRS; E. Covino (1); France); J.M. Alcal\'a (1); K. Biazzo (1); M. F. Sterzik (2)

arxiv: 1110.3712 · v1 · pith:6BUKFRNYnew · submitted 2011-10-17 · 🌌 astro-ph.SR

Large-scale young Gould Belt stars across Orion

K. Biazzo (1) , J.M. Alcal\'a (1) , M. F. Sterzik (2) , E. Covino (1) , A. Frasca (3) , P. Guillout (4) ((1) INAF - Capodimonte Astronomical Observatory , (2) European Southern Observatory (ESO) - Chile , (3) INAF - Catania Astrophysical Observatory

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(4) Observatoire Astronomique de Strasbourg CNRS France)

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keywords orionbeltgouldlarge-scaleacrossall-skycenteredclose

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We report first results on the large-scale distribution of the ROSAT All-Sky Survey (RASS) X-ray sources in a 5000 deg^2 field centered on Orion. Our final aim is to study the properties of different widespread populations in the Orion Complex close to the Gould Belt (GB) in order to trace the star formation history in the solar neighbourhood.

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Large-scale young Gould Belt stars across Orion

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