Computer Science – Sound
Scientific paper
Oct 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982stin...8314033s&link_type=abstract
Presented at the I.A.U. Symp. 101 Supernova Remnants and Their X-ray Emission, Venice, 30 Aug. - 2 Sep. 1982
Computer Science
Sound
Background Radiation, Diffuse Radiation, Supernova Remnants, X Ray Sources, Intergalactic Media, Power Spectra, Radiation Absorption, Rocket Sounding, Sky Radiation, Sun
Scientific paper
Almost all of the B band (0.10-0.19 keV) and C band (0.15-0.28 keV) X-rays probably originate in a hot region surrounding the Sun, which Cox and Anderson modeled as a supernova remnant. This same region may account for a significant fraction of the M band (0.5-1 keV) X-rays if the nonequilibrium models of Cox and Anderson are applicable. A population of distant SNR similar to the local region, with center-to-center spacing of about 300 pc, could provide enough galactic M band emission to fill in the dip in the count rate in the galactic plane that would otherwise be present due to absorption of both the extra galactic power law flux and any large-scale-height stellar (or galactic halo) emission.
Burrows David N.
Kraushaar William L.
McCammon Dan
Sanders Wilton T.
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