Enhanced Polarized Emission from the One-Parsec-Scale Hotspot of 3C 84 as a Result of the Interaction with Clumpy Ambient Medium
arXiv:1709.06708 · doi:10.3847/1538-4357/aa8e43
Abstract
We present Very Long Baseline Array polarimetric observations of the innermost jet of 3C84 (NGC1275) at 43GHz. A significant polarized emission is detected at the hotspot of the innermost re-started jet, which is located 1 pc south from the radio core. While the previous report presented a hotspot at the southern end of the western limb, the hotspot location has been moved to the southern end of the eastern limb. Faraday rotation is detected within an entire bandwidth of the 43-GHz band. The measured rotation measure (RM) is at most (6.31.9)radm and might be slightly time variable on the timescale of a month by a factor of a few. Our measured RM and the RM previously reported by the CARMA and SMA observations cannot be consistently explained by the spherical accretion flow with a power-law profile. We propose that a clumpy/inhomogeneous ambient medium is responsible for the observed rotation measure. Using equipartition magnetic field, we derive the electron density of cm. Such an electron density is consistent with the cloud of narrow line emission region around the central engine. We also discuss the magnetic field configuration from black hole scale to pc scale and the origin of low polarization.
8 pages, 8 figures, accepted for publication in ApJ
References in corpus (17)
- Heating Hot Atmospheres with Active Galactic Nuclei
- The Inner Jet of the Radio Galaxy M87
- Cold molecular gas in the Perseus cluster core - Association with X-ray cavity, Halpha filaments and cooling flow -
- Placing Confidence Limits on Polarization Measurements
- Magnetic support of the optical emission line filaments in NGC 1275
- Spine-sheath layer radiative interplay in subparsec-scale jets and the TeV emission from M87
- Magnetic Fields in the Center of the Perseus Cluster
- The Existence of Inner Cool Disks in the Low Hard State of Accreting Black Holes
- Radially-Inflowing Molecular Gas in NGC 1275 Deposited by a X-ray Cooling Flow in the Perseus Cluster
- The Mid-Infrared Emission of M87
- Magnetization degree at the jet base of M87 derived from the event horizon telescope data: Testing magnetically driven jet paradigm
- On the spine-layer scenario for the very high-energy emission of NGC 1275
- Discovery of a new subparsec counterjet in NGC 1275: the inclination angle and the environment
- Probing the Parsec-scale Accretion Flow of 3C 84 with Millimeter Polarimetry
- A Non-thermal Study of the Brightest Cluster Galaxy NGC 1275 - The Gamma-Radio Connection Over Four Decades
- Hitomi observations of Perseus support heating by mixing
- The Origin of Ripples in Cool Cores of Galaxy Clusters: Heating by MHD Waves?
Cited by in corpus (19)
- Polarimetric properties of Event Horizon Telescope targets from ALMA
- Faraday rotation in the jet of M87 inside the Bondi radius: indication of winds from hot accretion flows confining the relativistic jet
- Jet collimation in NGC 315 and other nearby AGN
- Ordered magnetic fields around the 3C 84 central black hole
- GPCAL: a generalized calibration pipeline for instrumental polarization in VLBI data
- RadioAstron discovery of a mini-cocoon around the restarted parsec-scale jet in 3C 84
- Jet kinematics in the transversely stratified jet of 3C 84 A two-decade overview
- The Dynamics and Energetics of Remnant and Restarting RLAGN
- A detailed kinematic study of 3C 84 and its connection to Gamma-rays
- Constraints on Circumnuclear Disk through Free-Free Absorption in the Nucleus of 3C 84 with KaVA and KVN at 43 and 86 GHz
- Evidence for a toroidal magnetic field in the core of 3C 84
- Polarization Observations of AGN Jets: Past and Future
- Diffuse Synchrotron Emission Associated with the Starburst in the Circumnuclear Disk of NGC 1275
- Probing the Heart of Active Narrow-line Seyfert 1 Galaxies with VERA Wideband Polarimetry
- Discovery of Radio Jets in Phoenix Galaxy Cluster Center
- Evolution, speed, and precession of the parsec-scale jet in the 3C 84 radio galaxy
- The Japanese Vision for the Black Hole Explorer Mission
- A revised view of the linear polarization in the subparsec core of M87 at 7 mm
- Where within the 3C 84 jet are -rays produced?