The relationship between X-ray variability and the central black hole mass
Open Access
- 21 June 2001
- journal article
- research article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 324 (3) , 653-658
- https://doi.org/10.1046/j.1365-8711.2001.04344.x
Abstract
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This publication has 28 references indexed in Scilit:
- Black Hole Mass Estimates from Reverberation Mapping and from Spatially Resolved KinematicsThe Astrophysical Journal, 2000
- A Fundamental Relation between Supermassive Black Holes and Their Host GalaxiesThe Astrophysical Journal, 2000
- A Relationship between Nuclear Black Hole Mass and Galaxy Velocity DispersionThe Astrophysical Journal, 2000
- What Is the Accretion Rate in NGC 4258?The Astrophysical Journal, 1999
- A Cutoff in the X‐Ray Fluctuation Power Density Spectrum of the Seyfert 1 Galaxy NGC 3516The Astrophysical Journal, 1999
- The X‐Ray Spectral Variability of the Seyfert Galaxy NGC 3227The Astrophysical Journal, 1998
- Anticorrelation of Variability Amplitude with X-Ray Luminosity for Active Galactic NucleiThe Astrophysical Journal, 1996
- On the nature of rapid X-ray variability in active galactic nucleiMonthly Notices of the Royal Astronomical Society, 1993
- The emission-line properties of low-redshift quasi-stellar objectsThe Astrophysical Journal Supplement Series, 1992
- Limits of X-ray variability in active galactic nucleiNature, 1986