The virial mass distribution of ultradiffuse galaxies in clusters and groups
Author:
Affiliation:
1. Max Planck Institute for Astrophysics, Karl-Schwarzschild-Strasse 1, D-85748 Garching, Germany
2. Institute for Theory and Computation, Harvard–Smithsonian centre for Astrophysics, 60 Garden St, Cambridge, MA 02138, USA
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnrasl/article-pdf/475/1/L116/24841674/sly012.pdf
Reference46 articles.
1. A deep wide survey of faint low surface brightness galaxies in the direction of the Coma cluster of galaxies
2. Ultradiffuse galaxies: the high-spin tail of the abundant dwarf galaxy population
3. GLOBULAR CLUSTERS INDICATE THAT ULTRA-DIFFUSE GALAXIES ARE DWARFS
4. AN OVERMASSIVE DARK HALO AROUND AN ULTRA-DIFFUSE GALAXY IN THE VIRGO CLUSTER
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