We present early results of our multiwavelength study of the star forming region IRAS 20050+2720. While we use X-rays and IR to classify young stellar objects, the optical data can be used to exclude foreground objects. The dataset set contains 57 class I sources, 183 class II sources and 183 X-ray sources, of which 140 are class III candidates. Within IRAS 20050+2720 four subclusters are found. Subcluster A and B are the densest regions, which contain stars of all evolutionary stages. Subcluster C is much younger than the other two. It has not formed any class III objects yet. We newly identify a fourth subcluster, which consists mostly of class II objects and is located about 10 arcmin from the center of the cloud.
@article{arxiv.1012.1354,
title = {IRAS 20050+2720: Anatomy of a young stellar cluster},
author = {H. M. Guenther and S. J. Wolk and R. A. Gutermuth and B. Spitzbart and T. L. Bourke and I. Pillitteri and K. DeRose},
journal= {arXiv preprint arXiv:1012.1354},
year = {2015}
}