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
| Original language | English |
|---|---|
| Pages (from-to) | 184-191 |
| Number of pages | 8 |
| Journal | Galaxies |
| Volume | 3 |
| Issue number | 4 |
| DOIs | |
| Publication status | Published - 5 Nov 2015 |
Keywords
- astro-ph.GA
- astro-ph.CO
Fingerprint
Dive into the research topics of 'Tidal Dwarf Galaxies: Disc Formation at z=0'. Together they form a unique fingerprint.Cite this
- APA
- Author
- BIBTEX
- Harvard
- Standard
- RIS
- Vancouver