Exploring Accretion and Disk-Jet Connections in the LLAGN M81*
arXiv:1006.5755 · doi:10.1088/0004-637X/720/2/1033
Abstract
We report on a year-long effort to monitor the central supermassive black hole in M81 in the X-ray and radio bands. Using Chandra and the VLA, we obtained quasi-simultaneous observations of M81* on seven occasions during 2006. The X-ray and radio luminosity of M81* are not strongly correlated on the approximately 20-day sampling timescale of our observations, which is commensurate with viscous timescales in the inner flow and orbital timecales in a radially-truncated disk. This suggests that short-term variations in black hole activity may not be rigidly governed by the "fundamental plane", but rather adhere to the plane in a time-averaged sense. Fits to the X-ray spectra of M81* with bremsstrahlung models give temperatures that are inconsistent with the outer regions of very simple advection-dominated inflows. However, our results are consistent with the X-ray emission originating in a transition region where a truncated disk and advective flow may overlap. We discuss our results in the context of models for black holes accreting at small fractions of their Eddington limit, and the fundamental plane of black hole accretion.
Accepted for publication in ApJ
References in corpus (16)
- X-ray Properties of Black-Hole Binaries
- Relativistic X-ray Lines from the Inner Accretion Disks Around Black Holes
- A Long, Hard Look at the Low-Hard State in Accreting Black Holes
- The Fundamental Plane of Accretion Onto Black Holes with Dynamical Masses
- Black hole accretion disks in the canonical low-hard state
- Low-Luminosity Active Galactic Nuclei: Are They UV-Faint and Radio Loud?
- A Prominent Accretion Disk in the Low-Hard State of the Black Hole Candidate SWIFT J1753.5-0127
- Results from an extensive simultaneous broadband campaign on the underluminous active nucleus M81*: further evidence for mass-scaling accretion in black holes
- Evidence for a compact jet dominating the broadband spectrum of the black hole accretor XTE J1550-564
- Broadband X-ray Spectra of GX 339-4 and the Geometry of Accreting Black Holes in the Hard State
- Identification of black hole power spectral components across all canonical states
- Following the 2008 outburst decay of the black hole candidate H1743-322 in X-ray and radio
- Trapping of magnetic flux by the plunge region of a black hole accretion disk
- Kinematics of the Broad Line Region in M81
- Advection-dominated accretion, jets and the spectral energy distribution of LINERs
- CP-Violation in K, B and B_{s} decays
Cited by in corpus (17)
- The Relationship Between Black Hole Growth and Star Formation in Seyfert Galaxies
- Spectral Models for Low-luminosity Active Galactic Nuclei in LINERs: The Role of Advection-dominated Accretion and Jets
- Assessing luminosity correlations via cluster analysis: Evidence for dual tracks in the radio/X-ray domain of black hole X-ray binaries
- Broadband X-ray Spectra of the Ultraluminous X-ray Source Holmberg IX X-1 observed with NuSTAR, XMM-Newton and Suzaku
- Detection of jet precession in the active nucleus of M81
- X-ray Outflows and Super-Eddington Accretion in the Ultraluminous X-ray Source Holmberg IX X-1
- SWIFT J1910.2-0546: A possible black hole binary with a retrograde spin or truncated disk
- Fundamental Plane of Black Hole Activity in Quiescent Regime
- Discrete Knot Ejection from the Jet in a Nearby Low Luminosity Active Galactic Nucleus, M81*
- Bhjet: a public multi-zone, steady state jet + thermal corona spectral model
- The absence of a thin disc in M81
- An X-ray Census of Fast Radio Burst Host Galaxies: Constraints on AGN and X-ray Counterparts
- Nuclear Radio Jet from a Low-Luminosity Active Galactic Nucleus in NGC 4258
- A universal scaling law of black hole activity including gamma-ray bursts
- Ultra high energy cosmic rays and possible signature of black strings
- The X-ray variation of M81* resolved by Chandra and NuSTAR
- An Energetic Hot Wind from the Low-luminosity Active Galactic Nucleus M81*