A forming wide polar-ring galaxy at z ~ 0.05 in the VST Deep Field of the Fornax cluster

Journal
Date Issued
2015
Author(s)
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Capaccioli, M.
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Limatola, L.
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•
DOI
Description
We are very grateful to the anonymous referee for his or her comments and suggestions that helped us to improve and clarify our work. This work was supported by the PRIN-INAF “Galaxy Evolution with the VLT Survey Telescope (VST)” (PI A. Grado). M. Cantiello acknowledges support from PO FSE Abruzzo 2007-2013 (PO 2012/2013).
Abstract
We present the first deep photometry of what may be a good candidate for a forming polar-ring galaxy at redshift z ≃ 0.05. The object FCSS J033710.0-354727 is a background galaxy in the VST Deep Field of the Fornax cluster. The deep exposures combined with the high angular resolution of the OmegaCam at VST allowed us to carry out the first detailed photometric analysis for this system in the g and i bands to derive the galaxy structure and colors. Results show that the central object resembles a disk galaxy, surrounded by a ring-like structure that is twice as extended as the central disk. The warped geometry and bright knots observed along the polar direction, as well as some debris detected on the NW side with colors similar to those of the galaxy, suggest that the polar structure is still forming. We argue that the wide polar ring or disk is the result of the ongoing disruption of a companion galaxy in the potential well of the central object, which is two to three times more massive than the accreting galaxy.

This work is based on observations taken at the ESO La Silla Paranal Observatory within the VST GTO Program ID 088.B-4012(A).

Volume
574
Start page
A111
Uri
Url
Issn Identifier
0004-6361
Ads BibCode
2015A&A...574A.111I
Rights
open.access
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