Magnetic field studies in BL lacertae through faraday rotation and a novel astrometric technique

DOI: 
10.3390/galaxies5040097
Publication date: 
12/12/2017
Main author: 
Molina S.N.
IAA authors: 
Molina, S.N.;Gómez, J.L.
Authors: 
Molina S.N., Gómez J.L., Dodson R., Rioja M.J.
Journal: 
Galaxies
Publication type: 
Article
Volume: 
5
Number: 
97
Issue: 
4
Abstract: 
<p>It is thought that dynamically important helical magnetic fields twisted by the differential rotation of the black hole's accretion disk or ergosphere play an important role in the launching, acceleration, and collimation of active galactic nuclei (AGN) jets. We present multi-frequency astrometric and polarimetric Very Long Baseline Array (VLBA) images at 15, 22, and 43 GHz, as well as Faraday rotation analyses of the jet in BL Lacertae as part of a sample of AGN jets aimed to probe the magnetic field structure at the innermost scales to test jet formation models. The novel astrometric technique applied allows us to obtain the absolute position at mm wavelengths without any external calibrator. © 2017 by the authors.</p>
Database: 
SCOPUS
URL: 
https://www.scopus.com/inward/record.uri?eid=2-s2.0-85037723797&doi=10.3390%2fgalaxies5040097&partnerID=40&md5=fc0dc8526a68b43a177f3bc81b96732a
Keywords: 
Astrometry; Galaxies: active; Galaxies: individual (BL Lacertae); Galaxies: jets; Polarization