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Optical spectroscopy of young tidal objects around two interacting galaxy pairs
Journal article   Open access   Peer reviewed

Optical spectroscopy of young tidal objects around two interacting galaxy pairs

K. Lee-Waddell, J. P. Madrid, K. Spekkens, C. J. Donzelli, B. S. Koribalski, P. Serra and J. Cannon
Monthly notices of the Royal Astronomical Society, Vol.480(2), pp.2719-2725
10/01/2018
DOI: 10.1093/mnras/sty2042

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Abstract

We present Gemini Multi-Object Spectrograph spectra of HI-rich tidal features located around the outskirts of two interacting galaxy pairs, NGC 3166/9 and NGC 4725/47. These follow-up observations are part of a multiwavelength campaign to study the properties and frequency of tidal dwarf galaxies (TDGs) in group environments. Based on the calculated gas-phase metallicity and redshift, in addition to the previously measured H I( )and stellar properties, we have confirmed the tidal origins of TDG candidate AGC 208457, which has emerged from the tidal debris of an interaction between the NGC 3166/9 galaxy pair. By comparing H I and optical recessional velocities, we have also confirmed a physical association of the gaseous knots and star clusters embedded in the metal-rich tidal tail of NGC 4747.
Astronomy & Astrophysics Physical Sciences Science & Technology

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