A transition from parabolic to conical shape as a common effect in nearby AGN jets

Y Y Kovalev, A B Pushkarev, E E Nokhrina, A V Plavin, V S Beskin, A V Chernoglazov, M L Lister, Tuomas Savolainen

Research output: Contribution to journalArticleScientificpeer-review

12 Citations (Scopus)
16 Downloads (Pure)

Abstract

Observational studies of collimation in jets in active galactic nuclei (AGN) are a key to understanding their formation and acceleration processes. We have performed an automated search for jet shape transitions in a sample of 367 AGN using VLBA data at 15 and 1.4 GHz. This search has found 10 out of 29 nearby jets at redshifts z < 0.07 with a transition from a parabolic to conical shape, while the full analysed sample is dominated by distant AGN with a typical z ≈ 1. The ten AGN are UGC 00773, NGC 1052, 3C 111, 3C 120, TXS 0815−094, Mrk 180, PKS 1514+00, NGC 6251, 3C 371, and BL Lac. We conclude that the geometry transition may be a common effect in AGN jets. It can be observed only when sufficient linear resolution is obtained. Supplementing these results with previously reported shape breaks in the nearby AGN 1H 0323+342 and M87, we estimate that the break occurs at 10 5–10 6 gravitational radii from the nucleus. We suggest that the jet shape transition happens when the bulk plasma kinetic energy flux becomes equal to the Poynting energy flux, while the ambient medium pressure is assumed to be governed by Bondi accretion. In general, the break point may not coincide with the Bondi radius. The observational data support our model predictions on the jet acceleration and properties of the break point.

Original languageEnglish
Pages (from-to)3576-3591
Number of pages16
JournalMonthly Notices of the Royal Astronomical Society
Volume495
Issue number4
DOIs
Publication statusPublished - 2021
MoE publication typeA1 Journal article-refereed

Fingerprint Dive into the research topics of 'A transition from parabolic to conical shape as a common effect in nearby AGN jets'. Together they form a unique fingerprint.

Cite this