PKS2250-41: a case study for triggering
K. J. Inskip, M. Villar-Martin, C. N. Tadhunter, R. Morganti, J. Holt, and D. Dicken

TL;DR
This study investigates the complex gas kinematics and ionization in the extended emission line region of the radio galaxy PKS2250-41, providing evidence that galaxy interactions may trigger radio source activity.
Contribution
It offers a detailed multiwavelength analysis linking galaxy interactions to the activation of radio sources, highlighting the role of tidal structures and environmental factors.
Findings
EELR shows complex gas kinematics and ionization states.
Evidence of galaxy interactions potentially triggering radio activity.
Alignment of filamentary structures with companion galaxy supports interaction hypothesis.
Abstract
We present the results of a multiwavelength study of the z = 0.31 radio source PKS2250-41. Integral field unit and long-slit spectroscopy obtained using VIMOS and FORS1 on the VLT, and archival HST optical imaging observations are used to study the morphology, kinematics and ionisation state of the extended emission line region (EELR) surrounding this source, and also a companion galaxy at a similar redshift. Near-infrared imaging observations obtained using the NTT are used to analyse the underlying galaxy morphologies. The EELR displays a complex variety of different gas kinematics and ionization states, consistent with a mixture of radio source shocks and AGN photoionization. The radio galaxy is likely to lie within a group environment, and is plausibly undergoing interactions with one or more other objects. The disk-like galaxy to the northeast of the radio source lies at a similar…
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.
