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- W2065509808 abstract "Data from a recent lunar occultation show the existence of a soft, weak X-ray source close to or within the Crab Nebula. The interpretations of the data include a weak point source in the field of view, an extended source associated with the expanding filaments of the Crab, or the scattering of X-rays by interstellar dust between the Earth and the Crab. If these X-rays are associated with the ejected material from the Crab, then the X-ray nebular emission can be divided into two parts. One part is a strong source of approximately 2' diameter associated with and surrounding the pulsar and being decidedly nonthermal in nature, and a second part where a few percent of the Crab X-rays come from a larger region and are perhaps thermal. The luminosity and spectrum of this second ''thermal'' source is compatible with that of other young supernova remnants. This and the alternate interpretations of the data are considered, and useful information is derived. (AIP)" @default.
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- W2065509808 date "1976-07-01" @default.
- W2065509808 modified "2023-09-23" @default.
- W2065509808 title "Evidence for 'thermal' X-rays from the Crab Nebula" @default.
- W2065509808 doi "https://doi.org/10.1086/154471" @default.
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