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- W1657156732 abstract "It is often held that the X-ray emission from active galactic nuclei (AGN) arises from a region close to the central energy source. Thus X-ray observations may provide the best constraints on the central engine. In particular, the shape of the X-ray continuum gives information about the mechanism for photon generation, X-ray time variability data can constrain the size and mass of the continuum source, and X-ray occultation data give constraints on the relative sizes of the continuum source and the intervening absorbing material (often assumed to be the broad line clouds). In addition, since a fair fraction of the total energy of an AGN is emitted at X-ray wavelengths, direct measurement of the amount and spectral form of this radiation is important for modeling of the optically emitting clouds." @default.
- W1657156732 created "2016-06-24" @default.
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- W1657156732 date "1985-03-01" @default.
- W1657156732 modified "2023-09-27" @default.
- W1657156732 title "X-ray emission from active galactic nuclei" @default.
- W1657156732 hasPublicationYear "1985" @default.
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