THE INITIAL MASS FUNCTION OF THE ORION NEBULA CLUSTER ACROSS THE H-BURNING LIMIT

We present a new census of the Orion Nebula Cluster over a large field of view (gsim 30' × 30'), significantly increasing the known population of stellar and substellar cluster members with precisely determined properties. We develop and exploit a technique to determine stellar effective t...

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Bibliographic Details
Main Authors: Da Rio, N. (Author), Robberto, M. (Author), Hillenbrand, L. A. (Author), Henning, T. (Author), Stassun, Keivan (Contributor)
Other Authors: Massachusetts Institute of Technology. Department of Physics (Contributor)
Format: Article
Language:English
Published: Institute of Physics/American Astronomical Society, 2015-02-18T20:48:57Z.
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