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The structure of the local hot bubble toward l = 165°, b = 0° using IUE and ROSAT data

  • UV And Soft X-Ray Observations Of The LISM
  • Conference paper
  • First Online:
The Local Bubble and Beyond Lyman-Spitzer-Colloquium

Part of the book series: Lecture Notes in Physics ((LNP,volume 506))

Abstract

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.

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References

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Author information

Authors and Affiliations

  1. Sternwarte, Universität Bonn, Auf dem Hügel 71, D-53121, Bonn

    K. S. de Boer

  2. Radioastronomisches Institut, Univ. Bonn, Auf dem Hügel 71, D-53121, Bonn

    J. Kerp

Authors
  1. K. S. de Boer
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  2. J. Kerp
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Editor information

Dieter Breitschwerdt Michael Freyberg Joachim Trümper

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© 1998 Springer-Verlag

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de Boer, K.S., Kerp, J. (1998). The structure of the local hot bubble toward l = 165°, b = 0° using IUE and ROSAT data. In: Breitschwerdt, D., Freyberg, M., Trümper, J. (eds) The Local Bubble and Beyond Lyman-Spitzer-Colloquium. Lecture Notes in Physics, vol 506. Springer, Berlin, Heidelberg. https://doi.org/10.1007/BFb0104695

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  • DOI: https://doi.org/10.1007/BFb0104695

  • Published:

  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-540-64306-7

  • Online ISBN: 978-3-540-69726-8

  • eBook Packages: Springer Book Archive

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