Comparing young massive clusters and their progenitor clouds in the Milky Way
Young massive clusters (YMCs) have central stellar mass surface densities exceeding $10^{4} M_{\odot} pc^{-2}$. It is currently unknown whether the stars formed at such high (proto)stellar densities. We compile a sample of gas clouds in the Galaxy which have sufficient gas mass within a radius of a...
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| Main Authors: | , |
|---|---|
| Format: | Article (Journal) Chapter/Article |
| Language: | English |
| Published: |
2016
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| In: |
Arxiv
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| Online Access: | Verlag, kostenfrei, Volltext: http://arxiv.org/abs/1602.02762
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| Author Notes: | D.L. Walker, S.N. Longmore, N. Bastian, J.M.D. Kruijssen, J.M. Rathborne, R. Galván-Madrid, and H.B. Liu |
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