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A Search for Dense Gas Around Young Stars

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Submillimetre Astronomy

Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 158))

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Abstract

We searched for CS(7–6) emission in a range of young stars, to test for the presence of dense gas. CS emission was detected only towards high-luminosity objects. We suggest that this is because the low-luminosity objects cannot heat a sufficient volume of gas to produce detectable CS emission.

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References

  • Keene, J. B., and Masson, C. R. 1987, B.A.A.S., 18, 293.

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  • Mundy, L. G., Wilking, B. A., and Myers, S. T. 1986, Ap.J.(Letters), 311, L75. Sutton, E. C., Danchi, W., and Jaminet, P., 1988, in preparation.

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© 1990 Springer Science+Business Media Dordrecht

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Masson, C.R. et al. (1990). A Search for Dense Gas Around Young Stars. In: Watt, G.D., Webster, A.S. (eds) Submillimetre Astronomy. Astrophysics and Space Science Library, vol 158. Springer, Dordrecht. https://doi.org/10.1007/978-94-015-6850-0_101

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  • DOI: https://doi.org/10.1007/978-94-015-6850-0_101

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-015-6852-4

  • Online ISBN: 978-94-015-6850-0

  • eBook Packages: Springer Book Archive

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