Molecular Gas Around Young Stellar Clusters
Astrophysics
2007-05-23 v1
Abstract
We have begun a survey of the molecular gas surrounding 31 young clusters in order to investigate the link between environment and the resulting cluster. We present here a preliminary comparison of two clusters in our sample: GGD12-15 and Mon R2. Since both clusters are located in the MonR2 molecular cloud at a distance of 830 pc, observational biases due to differing sensitivities and angular resolutions are avoided.
Cite
@article{arxiv.astro-ph/0110297,
title = {Molecular Gas Around Young Stellar Clusters},
author = {Naomi A. Ridge and Tom Megeath and T. L. Wilson},
journal= {arXiv preprint arXiv:astro-ph/0110297},
year = {2007}
}
Comments
2 pages, 2 figures, uses newpasp.sty. To appear in "Hot Star Workshop III: The Earliest Phases of Massive Star Birth" (ed. P.A. Crowther)