Characterization of the Young Open Cluster G144.9+0.4 in the Camelopardalis OB1 Association
Abstract
Our star-count analysis of the Two Micron All Sky Survey point sources resulted in an identification of the star cluster G144.9+0.4. The cluster was found, but not characterized, by Glushkova et al. We show that the cluster is physically associated with the Cam OB1 association at a distance of about 1 kpc and with an age of 1-2 Myr. Pre-main sequence stars are identified on the basis of photometric and proper motion data. A total of 91 additional OB star candidates was found in subgroups 1A and 1B, a significant increase from the currently known 43 OB stars. The OB members show an age spread that indicates a sustained star formation for at least the last 10-15 Myr. The young cluster G144.9+0.4 represents the latest episode of sequential star formation in this cloud complex.
Keywords
Cite
@article{arxiv.1308.6162,
title = {Characterization of the Young Open Cluster G144.9+0.4 in the Camelopardalis OB1 Association},
author = {Chien-Cheng Lin and W. P. Chen and Neelam Panwar},
journal= {arXiv preprint arXiv:1308.6162},
year = {2015}
}
Comments
33pages, 10 figures, published in ApJ