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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

K.S. de Boer
Affiliation:
Sternwarte, Universität Bonn, Auf dem Hügel 71, D-53121 Bonn
J. Kerp
Affiliation:
Radioastronomisches Institut, Univ. Bonn, Auf dem Hügel 71, D-53121 Bonn

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
Copyright
Copyright © Springer-Verlag 1998

References

Pruscione, A., Hawkins, I., Jelinsky, P., Wiercigroch, A., 1994, ApJS 94, 127 CrossRefGoogle Scholar
Hartmann, D., Burton, W.B., 1997, ‘An Atlas of Galactic Neutral Hydrogen’. Cam-bride University Press Google Scholar
Lilienthal, D., de Boer, K.S., 1991, A&AS 87, 471 Google Scholar