Modeling Water Emission from Intermediate Mass Star Formation Regions
In this research water emission is modeled from intermediate mass star formations regions placed at 1 kpc. Nine models are created to describe these regions of varying source luminosity ($L=100,500,$ and $1000L_{\odot}$) and protostellar envelope mass ($M=10,100,$ and $500M_{\odot}$). For each model...
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| Language: | en |
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2008
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| Online Access: | http://hdl.handle.net/10012/3998 |