Observations of the Structure and Dynamics of the Inner M87 Jet

Bibliographic Details
Title: Observations of the Structure and Dynamics of the Inner M87 Jet
Authors: Walker, R. Craig, Hardee, Philip E., Davies, Fred, Ly, Chun, Junor, William, Mertens, Florent, Lobanov, Andrei
Source: Galaxies 2016, 4(4), 46
Publication Year: 2016
Collection: Astrophysics
Subject Terms: Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Astrophysics of Galaxies
More Details: M87 is the best source in which to study a jet at high resolution in gravitational units because it has a very high mass black hole and is nearby. The angular size of the black hole is second only to Sgr A*, which does not have a strong jet. The jet structure is edge brightened with a wide opening angle base and a weak counterjet. We have roughly annual observations for 17 years plus intensive monitoring at three week intervals for a year and five day intervals for 2.5 months made with the Very Long Baseline Array (VLBA) at 43 GHz. The inner jet shows very complex dynamics, with apparent motions both along and across the jet. Speeds from zero to over 2c are seen, with acceleration observed over the first 3 milli-arcseconds. The counterjet decreases in brightness much more rapidly than the main jet, as is expected from relativistic beaming in an accelerating jet oriented near the line-of-sight. Details of the structure and dynamics are discussed. The roughly annual observations show side-to-side motion of the whole jet with a characteristic time scale of about 9 years.
Comment: 11 pages, 7 figures. Published in a special issue of Galaxies which is the proceedings of "Blazars through Sharp Multi-Wavelength Eyes" edited by J. L. Gomez, A. P. Marscher, and S. G. Jorstad
Document Type: Working Paper
DOI: 10.3390/galaxies4040046
Access URL: http://arxiv.org/abs/1610.08600
Accession Number: edsarx.1610.08600
Database: arXiv
More Details
DOI:10.3390/galaxies4040046