Mass Function at the end of the Main Sequence: the M35 Open Cluster
Astrophysics
2009-10-31 v1
Abstract
We present very deep RIc photometry of the M35 open cluster. We have covered 30' \times 30', equivalent to about a fourth of the total area of the cluster. The data range from I_c=17.5 to 23.5 magnitudes, and the color interval is . Roughly, these values correspond from to in the cases of members of the cluster. By using the location of the stars on a Color-Magnitude Diagram, we have selected possible members of this cluster and obtained the Luminosity and Mass Functions of the M35 open cluster and compared them with those from the Pleiades.
Keywords
Cite
@article{arxiv.astro-ph/9905230,
title = {Mass Function at the end of the Main Sequence: the M35 Open Cluster},
author = {D. Barrado y Navascues and J. R. Stauffer and J. Bouvier and E. L. Martin},
journal= {arXiv preprint arXiv:astro-ph/9905230},
year = {2009}
}
Comments
4 pages. "Proceedings of the III Scientific Meeting of the Spanish Astronomical Society", 1999, Astrophysics and Space Sciences, in press