Warped polar ring in the Arp 212 galaxy
A.V. Moiseev (Special Astrophysical Observatory, Russia)

TL;DR
This study uses interferometry to analyze ionized gas kinematics in Arp 212, revealing a warped polar ring structure likely formed by gas accretion from a satellite galaxy.
Contribution
It provides detailed kinematic evidence of a warped polar ring in Arp 212, highlighting the galaxy's complex gas dynamics and formation history.
Findings
Discovery of two distinct ionized gas subsystems
Identification of a warped polar ring structure
Evidence of gas accretion from a satellite galaxy
Abstract
The Fabry-Perot scanning interferometer mounted on the 6-m telescope of the Special Astrophysical Observatory of the Russian Academy of Sciences is used to study the distribution and kinematics of ionized gas in the peculiar galaxy Arp 212 (NGC 7625, III Zw 102). Two kinematically distinct subsystems - the inner disk and outer emission filaments, are found within the optical radius of the galaxy. The first subsystem, at galactocentric distances r<3.5 kpc, rotates in the plane of the stellar disk. The inner part of the ionized-gas disk (r<1.5-2 kpc) exactly coincides with the previously known disk consisting of molecular gas. The second subsystem of ionized gas is located at galactocentric distances 2-6 kpc. This subsystem rotates in a plane tilted by a significant angle to the stellar disk. The angle of orbital inclination in the outer disk increases with galactocentric distance and…
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.
