Abstract
In this work we propose the Bardeen-Petterson effect as the mechanism for the jet precession in NGC 1275. To check if this is true we have estimated the angular momentum ratio and the alignment timescale predict by the theory and compared them with the numerical results presented in the literature. We were able to explain the precession period assuming an accretion disk with column surface density in the form of a power law with exponent 0.60.3.
Original language | English |
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Title of host publication | AGN WINDS IN CHARLESTON |
Editors | G Chartas, F Hamann, KM Leighly |
Place of Publication | SAN FRANCISCO |
Publisher | Astronomical Society of the Pacific |
Pages | 266-267 |
Number of pages | 2 |
ISBN (Print) | 978-1-58381-802-2 |
Publication status | Published - 2012 |
Event | Conference on AGN Winds in Charleston - Charleston, Seychelles Duration: 15 Oct 2011 → 18 Oct 2011 |
Publication series
Name | Astronomical Society of the Pacific Conference Series |
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Publisher | ASTRONOMICAL SOC PACIFIC |
Volume | 460 |
Conference
Conference | Conference on AGN Winds in Charleston |
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Country/Territory | Seychelles |
City | Charleston |
Period | 15/10/11 → 18/10/11 |
Keywords
- ACCRETION DISKS