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Comparison of celescope magnitudes with model atmosphere fluxes for A, F and G supergiantsComparison between theoretical colors calculated from model atmospheres and ultraviolet celescope observations of supergiant star atmospheres show that most stars are deficient in ultraviolet flux relative to theoretical models. It is concluded that not enough line blocking has been included in model atmospheres.
Document ID
19720024193
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Parsons, S. B. (Warner and Swasey Obs.)
Date Acquired
August 6, 2013
Publication Date
January 1, 1972
Publication Information
Publication: NASA, Washington The Sci. Results from the Orbiting Astron. Obs. (OAO-2)
Subject Category
Space Sciences
Accession Number
72N31843
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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IDRelationTitle19720024160Collected WorksThe scientific results from the Orbiting Astronomical Observatory (OAO-2)
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