Interstellar Dust Clouds
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Abstract
Using infrared observations of L1544, a dark cloud in the Taurus Molecular Complex, density maps were generated and the distribution was compared to that of a polytopic gas. A polytopic index of 3.5 was found to best fit the observed density distribution.
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Faculty mentor: Professor Terry Jones
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This research was supported by the Undergraduate Research Opportunities Program (UROP).
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Nolting, Chris. (2013). Interstellar Dust Clouds. Retrieved from the University Digital Conservancy, https://hdl.handle.net/11299/150107.
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