Light curve asymmetry of a relativistic accretion disk

Details Light curve asymmetry of a relativistic accretion disk Light curve asymmetry of a relativistic accretion disk

Jun 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987natur.327..600f&link_type=abstract

Nature (ISSN 0028-0836), vol. 327, June 18, 1987, p. 600, 601.

Astronomy and Astrophysics

Astrophysics

7

Accretion Disks, Asymmetry, Light Curve, Relativistic Plasmas, Stellar Models, Cataclysmic Variables, Continuous Radiation, Doppler Effect, Space-Time Functions, X Ray Sources

Scientific paper

The emergent radiation from accretion disks has been observed in several objects, and observational facts have confirmed and verified accretion disks in various astrophysical objects. To investigate accretion disks further, a strategy is proposed to search for and detect the peculiar properties of the emergent radiation from the inner region of a relativistic accretion disk around a compact object, that is, the asymmetric feature of light curves during the eclipse of the disk.

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