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Intensity Variations of the Soft X-ray Background: the Boundary Structure of the Local Hot Bubble at Low Galactic Latitudes
Published online by Cambridge University Press: 12 April 2016
Abstract
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42 ROSAT PSPC pointed observations in the Galactic plane (l ~ 4° – 26°) are mosaicked in order to study the spatial structure of the X-ray emitting gas in the Local Hot Bubble (LHB). Degree scale X-ray intensity variations are detected at the ±10% level in the ¼ keV band, which imply a likely influence from a clumpy boundary shell of the LHB in the observed ¼ keV band X-ray background. The possible origins of such a clumpy boundary structure of the LHB are discussed.
- Type
- Part VI Distant Hot Gas, SXRB Fluctuations, Dust, Gamma-rays
- Information
- International Astronomical Union Colloquium , Volume 166: The Local Bubble and Beyond , 1997 , pp. 325 - 328
- Copyright
- Copyright © Springer-Verlag 1998
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