Distribution of Young Stellar Populations in the Orion Region

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Scientific paper

Based on the survey of emission-line stars in a wide field of the Orion star forming region, surface distributions of young stellar populations and gaseous clouds are compared as a whole in an attempt to make a speculation on the star formation process in this region. Existence of a primeval molecular cloud is suggested as the birth site of older members of emission-line stars and probably of X-ray detected pre-main sequence stars.

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