Da Rio, N. and Robberto, M. and Hillenbrand, L. A. and Henning, T. and Stassun, K. G. (2012) The Initial Mass Function of the Orion Nebula Cluster Across the H-Burning Limit. Astrophysical Journal, 748 (1). Art. No. 14. ISSN 0004-637X http://resolver.caltech.edu/CaltechAUTHORS:20120418-071143101
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We present a new census of the Orion Nebula Cluster over a large field of view (≳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 temperatures from optical colors, nearly doubling the previously available number of objects with effective temperature determinations in this benchmark cluster. Our technique utilizes colors from deep photometry in the I band and in two medium-band filters at λ ~ 753 and 770 nm, which accurately measure the depth of a molecular feature present in the spectra of cool stars. From these colors we can derive effective temperatures with a precision corresponding to better than one-half spectral subtype, and importantly this precision is independent of the extinction to the individual stars. Also, because this technique utilizes only photometry redward of 750 nm, the results are only mildly sensitive to optical veiling produced by accretion. Completing our census with previously available data, we place some 1750 sources in the Hertzsprung-Russell diagram and assign masses and ages down to 0.02 solar masses. At faint luminosities, we detect a large population of background sources which is easily separated in our photometry from the bona fide cluster members. The resulting initial mass function of the cluster has good completeness well into the substellar mass range, and we find that it declines steeply with decreasing mass. This suggests a deficiency of newly formed brown dwarfs in the cluster compared to the Galactic disk population.
|Additional Information:||© 2012 American Astronomical Society. Received 2011 September 11; accepted 2011 December 12; published 2012 February 29. The authors acknowledge the Max-Planck Society (MPG) and the Max-Planck Institute for Astronomy (Heidelberg, Germany) for the telescope time. The IMF research of Thomas Henning is supported by Sonderforschungsbereich SFB 881 “The Milky Way System” (subproject B6) of the German Research Foundation (DFG). Facilities: Max Planck:2.2m, HST|
|Subject Keywords:||brown dwarfs; Hertzsprung-Russell and C-M diagrams; open clusters and associations: individual (Orion); stars: formation; stars: luminosity function, mass function; stars: pre-main sequence|
|Official Citation:||The Initial Mass Function of the Orion Nebula Cluster across the H-burning Limit N. Da Rio et al. 2012 ApJ 748 14|
|Usage Policy:||No commercial reproduction, distribution, display or performance rights in this work are provided.|
|Deposited By:||Ruth Sustaita|
|Deposited On:||18 Apr 2012 14:42|
|Last Modified:||26 Dec 2012 15:04|
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