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Circumstellar dust model for infrared stars

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Abstract

The expected thermal emission from the shell around stars has been calculated on the graphite model. The calculated spectral distribution is in reasonable agreement with the observed infrared emission from some of the infrared stars.

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Author notes

  1. K. S. Krishna Swamy

    Present address: Tata Institute of Fundamental Research, Colaba, Bombay 5, India

Authors and Affiliations

  1. Department of Space Science, Rice University, Houston, Texas, USA

    K. S. Krishna Swamy

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  1. K. S. Krishna Swamy
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Swamy, K.S.K. Circumstellar dust model for infrared stars. Astrophys Space Sci 9, 123–127 (1970). https://doi.org/10.1007/BF00649958

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  • DOI: https://doi.org/10.1007/BF00649958

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