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Small-Scale ¼ keV Fluctuations Due to the Local Hot Bubble
Published online by Cambridge University Press: 12 April 2016
Abstract
To determine fluctuations in the ¼ keV emission due to the LHB, without contamination due to sources within the galactic disk, the Galactic halo or the extragalactic background, we have formed a mosaic of PSPC observations towards the Hyades, a direction where distant emission is effectively blocked by a Galactic column of many optical depths. After removing the point sources from this image, we find the ¼ keV emission to be smooth on scales from 6′ to a few degrees.
- 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. 329 - 332
- Copyright
- Copyright © Springer-Verlag 1998