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- W1969006979 abstract "The solid state spectrometer on the Einstein Observatory and the GSFC cosmic X-ray spectrometer on OSO-8 observed the X-ray spectrum of SN1006. The data can be well-represented by a power-law model with alpha = 1.2, similar to the spectrum of the Crab nebula. This is in contrast to the radio and X-ray maps of SN1006 which show a shell structure more typical of SNR with thermal X-ray emission. The X-ray spectrum is suggestive of nonthermal synchrotron emission, raising the possibility that the remnant of SN1006 contains a source of relativistic electrons." @default.
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- W1969006979 date "1980-05-01" @default.
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- W1969006979 title "Is the remnant of SN1006 crab-like?" @default.
- W1969006979 hasPublicationYear "1980" @default.
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