ARE THE VARIATIONS IN QUASAR OPTICAL FLUX DRIVEN BY THERMAL FLUCTUATIONS?
BCBrandon C. KellyJBJill BechtoldASAneta Siemiginowska
University of Arizona · Center for Astrophysics Harvard & Smithsonian
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Abstract
We analyze a sample of optical light curves for 100 quasars, 70 of which have black hole mass estimates. Our sample is the largest and broadest used yet for modeling quasar variability. The sources in our sample have z
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Authors
3- BCBrandon C. KellyCorresponding
University of Arizona, Center for Astrophysics Harvard & Smithsonian
- JBJill Bechtold
University of Arizona
- ASAneta Siemiginowska
Center for Astrophysics Harvard & Smithsonian
Topics & keywords
Topics
Keywords
- Quasar
- Light curve
- Amplitude
- Flux (metallurgy)
- Black hole (networking)
- Thermal
- Scale (ratio)
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