Statistics – Computation
Scientific paper
Mar 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...338...32c&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 338, March 1, 1989, p. 32-36.
Statistics
Computation
22
Accretion Disks, Active Galactic Nuclei, Black Holes (Astronomy), Computational Astrophysics, Dwarf Novae, Ionization, Spectral Energy Distribution, Stellar Luminosity, Stellar Mass Accretion, Thermal Instability
Scientific paper
Thermal limit cycles in accretion disks are a promising explanation of the quasi-periodic outbursts of dwarf novae. A similar mechanism may lead to observable light variations in active galactic nuclei (AGNs) at wavelengths 1-5 microns. The variations should obey a characteristic period-luminosity relation. For low-luminosity AGNs, these variations could have a period of less than about 10 yr.
Clarke Catherine J.
Shields Gregory A.
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