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 ([> ~]30' x 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 effectiv...

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Veröffentlicht in:	The Astrophysical journal 2012-03, Vol.748 (1), p.1-15
Hauptverfasser:	DA RIO, N, ROBBERTO, M, HILLENBRAND, L. A, HENNING, T, STASSUN, K. G
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomy ASTROPHYSICS, COSMOLOGY AND ASTRONOMY Brown dwarf stars Census Clusters Cool stars Earth, ocean, space Exact sciences and technology HERTZSPRUNG-RUSSELL DIAGRAM Initial mass function LUMINOSITY MASS NEBULAE Orion nebula PHOTOMETRY Spectra STAR EVOLUTION STARS
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