http://arxiv.org/abs/1506.08034
We present observations of a 4 squared degree area toward the Gemini cloud obtained using J = 1-0 transitions of $^{12}$CO, $^{13}$CO and C$^{18}$O. No C$^{18}$O emission was detected. This region is composed of 36 core candidates of $^{13}$CO. These core candidates have a characteristic diameter of 0.25 pc, excitation temperatures of 7.9 K, line width of 0.54 km s$^{-1}$ and a mean mass of 1.4 M$_{\sun}$. They are likely to be starless core candidates, or transient structures, which probably disperse after $\sim$10$^6$ yr.
Y. Li, Y. Xu, J. Yang, et. al.
Mon, 29 Jun 15
17/41
Comments: Accepted for Publication in AJ, 23 Pages, 15 figures. arXiv admin note: text overlap with arXiv:astro-ph/0604427 by other authors
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