The Warped Disc of NGC 4258
arXiv:0804.1013 · doi:10.1111/j.1365-2966.2008.13275.x
Abstract
We consider the properties of the warped accretion disc in NGC 4258 which is delineated by maser emission. We use our analytical models to consider whether the disc could be warped by Lense-Thirring precession. We show that such models fit the shape of the disc well and we determine the goodness of fit for various combinations of the warp radius and the disc and black hole configurations. Though the fits are compelling evidence, we note that such a model has implications for the formation and longevity of the disc which might be problematic for the current understanding of Seyfert Galaxies.
Accepted for publication in MNRAS
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- Misalignment of the microquasar V4641 Sgr (SAX J1819.3--2525)
- A Survey of Satellite Galaxies around NGC 4258
- A fully relativistic twisted disk around a slowly rotating Kerr black hole: derivation of dynamical equations and the shape of stationary configurations
- High-redshift SMBHs can grow from stellar-mass seeds via chaotic accretion
- Warping of accretion disk and launching of jet by a spinning black hole in NGC 4258
- Toward the Gravitational Redshift Detection in NGC 4258 and the Estimation of its Black Hole Mass-to-Distance Ratio
- The torquing of circumnuclear accretion disks by stars and the evolution of massive black holes
- On Estimating the Mass of Keplerian Accretion Disks in H2O Maser Galaxies
- Accretion disk warping by resonant relaxation: The case of maser disk NGC4258
- Steady state solution of warped accretion discs
- Strong field effects on emission line profiles: Kerr black holes and warped accretion disks
- On the possibility of a warped disc origin of the inclined stellar discs at the Galactic Centre
- Analytical models of relativistic accretion disks
- Constraining the evolution of the unstable accretion disk in SMC X-1 with NICER
- Circum-nuclear molecular disks: role in AGN fueling and feedback
- Signatures of supermassive black hole binaries on maser systems