University of Hertfordshire

Tidal Dwarf Galaxies: Disc Formation at z=0

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Original languageEnglish
Number of pages8
Pages (from-to)184-191
JournalGalaxies
Journal publication date5 Nov 2015
Volume3
Issue4
DOIs
StatePublished - 5 Nov 2015

Abstract

Collisional debris around interacting and post-interacting galaxies often display condensations of gas and young stars that can potentially form gravitationally bound objects: Tidal Dwarf Galaxies (TDGs). We summarise recent results on TDGs, which are originally published in Lelli et al. (2015, A

Notes

This is a brief summary of arXiv:1509.05404, written for the Proceedings of the EWASS-2015 Special Session 3 "3D View on Interacting and Post-Interacting Galaxies from Clusters to Voids". © 2015 by the authors; licensee MDPI, Basel, Switzerland. This article is an open access article distributed under the terms and conditions of the Creative Commons Attribution license (http://creativecommons.org/licenses/by/4.0/).

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