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...
| Váldodahkkit: | , , , , |
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| Eará dahkkit: | |
| Materiálatiipa: | Artihkal |
| Giella: | en_US |
| Almmustuhtton: |
Institute of Physics/American Astronomical Society
2015
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| Liŋkkat: | http://hdl.handle.net/1721.1/94617 |