Discovery of a Flat-Spectrum Radio Nucleus in NGC 3115
arXiv:1209.6602 · doi:10.1088/0004-6256/144/6/160
Abstract
The early-type galaxy NGC 3115, at a distance of 10.2 Mpc, hosts the nearest billion-solar-mass black hole. Wong et al. recently inferred a substantial Bondi accretion rate near the black hole. Bondi-like accretion is thought to fuel outflows, which can be traced through their radio emission. This paper reports the discovery of a radio nucleus in NGC 3115, with a diameter less that 0.17 arcsec (8.4 pc), a luminosity at 8.5 GHz of 3.1 x 10^35 ergs/s and a flat spectrum (alpha = -0.23+/-0.20, flux density ~ frequency^alpha). The radio source coincides with the galaxy's photocenter and candidate X-ray nucleus. The emission is radio-loud, suggesting the presence of an outflow on scales less than 10 pc. On such scales, the Bondi accretion could be impeded by heating due to disruption of the outflow.
4 pages; 1 figure; emulateapj.cls; to appear in AJ
References in corpus (4)
Cited by in corpus (13)
- The Local Nanohertz Gravitational-Wave Landscape From Supermassive Black Hole Binaries
- Exploring the mass assembly of the early-type disc galaxy NGC3115 with MUSE
- The Megasecond Chandra XVP Observation of NGC 3115: Witnessing the Flow of Hot Gas within the Bondi Radius
- A Multi-wavelength Study of the Turbulent Central Engine of the Low-mass AGN hosted by NGC404
- Fundamental Plane of Black Hole Activity in Quiescent Regime
- An off-centered active galactic nucleus in NGC 3115
- The multiwavelength spectrum of NGC 3115: Hot accretion flow properties
- Recovering the origins of the lenticular galaxy NGC 3115 using multi-band imaging
- Modeling Hot Gas Flow in the Low-Luminosity Active Galactic Nucleus of NGC3115
- Suppressing hot gas accretion to supermassive black holes by stellar winds
- Hot Gas Flows on Parsec Scale in the Low-Luminosity Active Galactic Nucleus NGC 3115
- Investigating the Candidate Displaced Active Galactic Nucleus in NGC 3115
- Evaluating the efficacy of a data cube treatment procedure for kinematic analyses: application to NGC 3115 and NGC 4699