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Description
Theoretical spectral energy distributions (SEDs) from expanding NLTE model atmospheres for hot stars.
Keywords
Stellar atmospheres
Radiative transfer
Creator
Wolf-Rainer Hamann
Created
2013-03-14T13:25:52Z
Metadata updated
2020-09-17T08:06:17Z
Reference URL
http://www.astro.physik.uni-potsdam.de/~PoWR
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Information on resource 'PoWR'
Theoretical spectral energy distributions (SEDs) from expanding NLTE model atmospheres for hot stars.
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