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The Infrared Excess From Stellar Winds

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Light on Dark Matter

Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 124))

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Abstract

The IR excess can be used to study the density or velocity structure in the lower parts of the winds of early type stars. The depth of the emitting region and the excess in magnitudes is given for typical O-stars, as a function of λ and Ṁ. The first results of an ongoing study of the IRAS data are discussed briefly.

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© 1986 D. Reidel Publishing Company

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Lamers, H.J.G.L.M. (1986). The Infrared Excess From Stellar Winds. In: Israel, F.P. (eds) Light on Dark Matter. Astrophysics and Space Science Library, vol 124. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-4672-9_14

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  • DOI: https://doi.org/10.1007/978-94-009-4672-9_14

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-8577-9

  • Online ISBN: 978-94-009-4672-9

  • eBook Packages: Springer Book Archive

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