Modeling the Near-Infrared Luminosity Functions of Young Stellar Clusters
Abstract
We present the results of numerical experiments designed to evaluate the usefulness of near-infrared luminosity functions for constraining the Initial Mass Function (IMF) of young stellar populations. From this numerical modeling, we find that the luminosity function of a young stellar population is considerably more sensitive to variations in the underlying initial mass function than to either variations in the star forming history or assumed pre-main-sequence (PMS) mass-to-luminosity relation. To illustrate the potential effectiveness of using the KLF of a young cluster to constrain its IMF, we model the observed K band luminosity function of the nearby Trapezium cluster. Our derived mass function for the Trapezium spans two orders of magnitude in stellar mass (5 Msun to 0.02 Msun), has a peak near the hydrogen burning limit, and has an IMF for Brown Dwarfs which steadily decreases with decreasing mass.
Keywords
Cite
@article{arxiv.astro-ph/9912384,
title = {Modeling the Near-Infrared Luminosity Functions of Young Stellar Clusters},
author = {August A. Muench and Elizabeth A. Lada and Charles J. Lada},
journal= {arXiv preprint arXiv:astro-ph/9912384},
year = {2009}
}
Comments
To appear in ApJ (1 April 2000). 37 pages including 11 figures, AAS: ver 5.0