High altitude molecular clouds

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High Altitude Molecular Clouds

A population of molecular clouds with a significantly greater scale height than that of Giant Molecular Clouds has been identified by examining maps of the latitude distribution of the CO(1 − 0) emission in the first quadrant of the Galaxy. These clouds are found by identifying emission more than 2.6 times the scale-height away from the galactic midplane (centroid of CO emission) at the tangent...

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ژورنال

عنوان ژورنال: The Astrophysical Journal

سال: 1994

ISSN: 0004-637X,1538-4357

DOI: 10.1086/174988