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The Structure of the Local Hot Bubble Toward l = 165°, b = 0° Using IUE and ROSAT Data
Published online by Cambridge University Press: 12 April 2016
Abstract
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The first X-ray-opaque cloud in the direction of Auriga lies at 180 pc. A tenuous cloud, whose distance is derived from IUE absorption line studies as well as from an analysis of ROSAT data, is embedded at 55 pc. The X-ray emitting gas has a temperature of 105.9−6.0 K. The pressure is 1.6 104 K cm−3.
- Type
- Part II UV and Soft X-ray Observations of the LISM
- Information
- International Astronomical Union Colloquium , Volume 166: The Local Bubble and Beyond , 1997 , pp. 65 - 68
- Copyright
- Copyright © Springer-Verlag 1998
References
Pruscione, A., Hawkins, I., Jelinsky, P., Wiercigroch, A., 1994, ApJS
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