Soft X-ray Emission from the Vela Supernova Remnant
A soft X-ray observation of the Vela Supernova Remnant is described. X-ray surface brightness maps of the Remnant are presented in three energy intervals, 0.15 - 0.5 keV, 0.5 - 1.0 keV, and 1.0 - 2.0 keV, and in two different spatial resolutions, 1° x 1°, and 40' x 40'. The maps show a...
Internet
https://thesis.library.caltech.edu/10116/8/Moore_WE_1976.pdfMoore, William Edwin (1976) Soft X-ray Emission from the Vela Supernova Remnant. Dissertation (Ph.D.), California Institute of Technology. doi:10.7907/CH0R-SF30. https://resolver.caltech.edu/CaltechTHESIS:03292017-094816214 <https://resolver.caltech.edu/CaltechTHESIS:03292017-094816214>