NGC922 - A new drop-through ring galaxy
arXiv:astro-ph/0605613 · doi:10.1111/j.1365-2966.2006.10589.x
Abstract
We have found the peculiar galaxy NGC922 to be a new drop-through ring galaxy using multi-wavelength (UV-radio) imaging and spectroscopic observations. Its `C'-shaped morphology and tidal plume indicate a recent strong interaction with its companion which was identified with these observations. Using numerical simulations we demonstrate that the main properties of the system can be generated by a high-speed off-axis drop-through collision of a small galaxy with a larger disk system, thus making NGC922 one of the nearest known collisional ring galaxies. While these systems are rare in the local Universe, recent deep HST images suggest they were more common in the early Universe.
5 pages, accepted for publication in MNRAS Letters
References in corpus (9)
- The Optical and Near-Infrared Properties of Galaxies: I. Luminosity and Stellar Mass Functions
- Secular Evolution and the Formation of Pseudobulges in Disk Galaxies
- Using Strong Lines to Estimate Abundances in Extragalactic HII Regions and Starburst Galaxies
- The HIPASS Catalogue - I. Data Presentation
- The 6dF Galaxy Survey: Samples, Observational Techniques and the First Data Release
- The 1000 Brightest HIPASS Galaxies: HI Properties
- Galaxy Morphologies in the Hubble Ultra Deep Field: Dominance of Linear Structures at the Detection Limit
- The Luminosity-Metallicity relation in the local universe from the 2dF Galaxy Redshift Survey
- Lopsided spiral galaxies: evidence for gas accretion
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- Rings and Bent Chain Galaxies in the GEMS and GOOD Fields
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- The Star Cluster Population of the Collisional Ring Galaxy NGC 922
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- The host galaxy of GRB 980425 / SN1998bw: a collisional ring galaxy
- A giant umbrella-like stellar stream around the tidal ring galaxy NGC 922
- The X-Ray Luminosity Function of Ultra Luminous X-Ray Sources in Collisional Ring Galaxies
- Propagating Star Formation in the Collisional Ring Galaxy Arp 10
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- Chandra Observations of the Collisional Ring Galaxy NGC 922
- Stellar tidal streams around nearby spiral galaxies with deep imaging from amateur telescopes
- Early Science with the Large Millimeter Telescope: discovery of the 12CO(1-0) emission line in the ring galaxy, VIIZw466
- Formation of collisional ring galaxies in Milgromian dynamics
- Massive star clusters and clumps in the collisional ring galaxy Arp 147
- Young Stellar Populations in the Collisional Ring Galaxy NGC 922