Infrared Emission from Outflows Associated with Young Stars

Clark, F. O.; Laureijs, R. J.; Zhang, C. Y.; Chlewicki, G.; Wesselius, P. R.

doi:10.1007/978-94-009-2941-8_40

F. O. Clark^3,4,
R. J. Laureijs³,
C. Y. Zhang^3,5,
G. Chlewicki³ &
…
P. R. Wesselius³

Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 142))

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Abstract

The extended infrared emission detected near many young stars can be used to divine the luminosity, apparent color temperature, and thermal emitting mass of the surrounding regions. The dominant dust heating mechanism appears to be ultraviolet radiation, either from stellar wind shocks or directly from hotter stars. The infrared luminosities from stellar winds of low mass stars are an appreciable fraction of the luminosities of the driving star, and the mechanical luminosity in the winds must be even higher.

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Authors and Affiliations

Laboratory for Space Research Groningen, The Netherlands
F. O. Clark, R. J. Laureijs, C. Y. Zhang, G. Chlewicki & P. R. Wesselius
University of Kentucky, Lexington, KY, USA
F. O. Clark
Purple Mountain Obs., Academica Sinica, Nanjing, China
C. Y. Zhang

Authors

F. O. Clark
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R. J. Laureijs
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C. Y. Zhang
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G. Chlewicki
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P. R. Wesselius
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Editors and Affiliations

Osservatorio Astronomico di Torino, Pino Torinese, Italy
Luciana Bianchi
ESA/VILSPA, IUE Groundstation, Madrid, Spain
Roberto Gilmozzi

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Clark, F.O., Laureijs, R.J., Zhang, C.Y., Chlewicki, G., Wesselius, P.R. (1988). Infrared Emission from Outflows Associated with Young Stars. In: Bianchi, L., Gilmozzi, R. (eds) Mass Outflows from Stars and Galactic Nuclei. Astrophysics and Space Science Library, vol 142. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-2941-8_40

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DOI: https://doi.org/10.1007/978-94-009-2941-8_40
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-7824-5
Online ISBN: 978-94-009-2941-8
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