A Potential Galaxy Threshing System in the Cosmos Field

Abstract

We report on the discovery of a new potential galaxy threshing system in the COSMOS 2 square degree field using the prime-focus camera, Suprime-Cam, on the 8.2 m Subaru Telescope. This system consists of a giant elliptical galaxy with $M_V\approx -21.6$ and a tidally disrupted satellite galaxy with $M_V\approx -17.7$ at a photometric redshift of $z\approx 0.08$. This redshift is consistent with the spectroscopic redshift of 0.079 for the giant elliptical galaxy obtained from the Sloan Digital Sky Survey (SDSS) archive. The luminosity masses of the two galaxies are $3.7\times 10^{12}{\mathcal{M}}_{\odot }$ and $3.1\times 10^9{\mathcal{M}}_{\odot }$, respectively. The distance between the two galaxies is greater than 100 kpc. The two tidal tails emanating from the satellite galaxy extend over 150 kpc. This system would be the second well-defined galaxy threshing system found so far.

17 pages, 7 figures, accepted for the COSMOS special issue of ApJS

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Cited by in corpus (7)

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• Tidal streams around galaxies in the SDSS DR7 archive
• The Next Generation Virgo Cluster Survey. IV. NGC 4216: A Bombarded Spiral in the Virgo Cluster
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