Relativistic Doppler beaming and misalignments in AGN jets
Ashok K. Singal

TL;DR
This paper investigates how relativistic Doppler beaming and geometrical projection effects influence the brightness and apparent misalignments of jets in active galactic nuclei, highlighting the importance of orientation angles.
Contribution
It provides a detailed analysis of how projection effects can mimic large jet misalignments and predicts significant brightness contrasts due to relativistic beaming.
Findings
Large brightness ratios are expected before and after jet misalignments.
Projection effects can cause small intrinsic angle changes to appear as large misalignments.
Relativistic beaming significantly impacts observed jet brightness and structure.
Abstract
Radio maps of AGNs often show linear features, called jets, both on pc as well as kpc scales. These jets supposedly possess relativistic motion and are oriented close to the line of sight of the observer and accordingly the relativistic Doppler beaming makes them look much brighter than they really are in their respective rest-frames. The flux boosting due to the relativistic beaming is a very sensitive factor of the jet orientation angle, as seen by the observer. Quite often large bends are seen in these jets, with misalignments being or more and might imply a change in the orientation angle that could cause a large change in the relativistic beaming factor. Such large bends should show high contrasts in the brightness of the jets, before and after the misalignments, if relativistic beaming does play an important role in these jets. It needs to be kept in mind that sometimes…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
