UGC 4599: A Photometric Study of the Nearest Hoag-Type Ring Galaxy
arXiv:1102.3184 · doi:10.1111/j.1365-2966.2011.18330.x
Abstract
We present a photometric study of UGC 4599, a low-luminosity galaxy superficially resembling Hoag's Object in that on sky survey images it appears to be a complete ring surrounding a roundish core. The nature of the outer ring of Hoag-type galaxies is still debated and may be related either to slow secular evolution or to environmental processes, such as galaxy-galaxy interactions. we show that in UGC 4599 (a) the nearly round central body follows well an r^1/4 light profile almost all the way to the centre, (b) the isophotes are strongly twisted with a sharp 45 deg transition at a radius of r~6 arcsec, (c) the blue ring seems to have reached near-equilibrium configuration with the central body, (d) the ring is actually composed of a one-and-a-half turn spiral feature, and (e) one side of the spiral shows conspicuous star formation in the form of at least nine HII regions, revealed by their H_alpha emission. Based on the photometric data, together with HI information from the literature, we characterize UGC 4599 as an elliptical-like object surrounded by a luminous ring and a massive, extremely extended HI disc. Given its observed properties, we rule out UGC 4599 as representing a late phase in barred early-type galaxies evolution. We discuss the origin of UGC 4599 and conclude that this galaxy could be the result of a major interaction between two gas-rich spiral galaxies that took place at least 5 Gyr ago. However, deep optical imaging and a detailed stellar population analysis are required to determine whether the large gas reservoir could have been accreted directly from the intergalactic medium onto a pre-existing elliptical galaxy in the early Universe. A detailed kinematical study will shed light on the exact nature of the central body and the ring of UGC 4599.
14 pages, 6 figures and 5 tables. Accepted for publication in MNRAS. The abstract is abridged compared to the published version
References in corpus (16)
- UV Star Formation Rates in the Local Universe
- Star formation efficiency in galaxy interactions and mergers: a statistical study
- A Search for Extended Ultraviolet Disk (XUV-disk) Galaxies in the Local Universe
- The Structure of Classical Bulges And Pseudobulges: The Link Between Pseudobulges And Sersic Index
- Multiple minor mergers: formation of elliptical galaxies and constraints for the growth of spiral disks
- Neutral hydrogen in nearby elliptical and lenticular galaxies: the continuing formation of early-type galaxies
- Stellar populations of early-type galaxies in different environments II. Ages and metallicities
- Properties of Bars and Bulges in the Hubble Sequence
- The Westerbork Hydrogen Accretion in Local Galaxies (HALOGAS) Survey I. Survey Description and Pilot Observations
- The Northern HIPASS catalogue - Data presentation, completeness and reliability measures
- The mass-metallicity gradient relation of early-type galaxies
- Extended, regular HI structures around early-type galaxies
- Stellar populations, neutral hydrogen and ionised gas in field early-type galaxies
- The role of spin in the formation and evolution of galaxies
- IC 4200: a gas-rich early-type galaxy formed via a major merger
- Galaxy mergers at high resolution: From elliptical galaxies to tidal dwarfs and globular clusters
Cited by in corpus (10)
- A new catalogue of polar-ring galaxies selected from the SDSS
- HIghMass -- High HI Mass, HI-rich Galaxies at z~0: Sample Definition, Optical and Halpha Imaging, and Star Formation Properties
- Hoag's Object: Evidence for Cold Accretion onto an Elliptical Galaxy
- The galaxy population within the virial radius of the Perseus cluster
- The H Dots Survey. II. A Second List of Faint Emission-Line Objects
- Lenticular galaxies with UV-rings
- A photometric study of the peculiar and potentially double ringed, non-barred galaxy: PGC 1000714
- Star Formation in Outer Rings of S0 galaxies. V. UGC 4599 -- an S0 with gas probably accreted from a filament
- The structure and stability of orbits in Hoag-like ring systems
- DES J024008.08-551047.5:A new member of the polar ring galaxy family