A List of Dwarf Galaxies in the Local Supercluster
D. Makarov, and R. Uklein. (2012)cite arxiv:1204.5406Comment: 17 pages, 6 figures, 2 tables, to be published in Astrophysical Bulletin 67, p.123 (2012).
DOI: 10.1134/S1990341312020010
Abstract
We report a list of groups consisting of dwarf galaxies only. The sample
contains 126 objects, mainly combined in pairs. The most populated group
contains six dwarf galaxies. The majority of systems considered reside in the
low-density regions and evolve unaffected by massive galaxies. The
characteristic sizes and velocity dispersions of groups are 30 kpc and 11 km/s,
respectively. They resemble the associations of dwarf galaxies, but are more
compact. On the whole, groups and associations form a continuous sequence.
Alike the associations, our groups possess high mass-to-luminosity ratios, what
is indicative of a large amount of dark matter present in these systems.
Description
[1204.5406] A List of Dwarf Galaxies in the Local Supercluster
%0 Generic
%1 makarov2012dwarf
%A Makarov, D. I.
%A Uklein, R. I.
%D 2012
%K catalogue galaxy
%R 10.1134/S1990341312020010
%T A List of Dwarf Galaxies in the Local Supercluster
%U http://arxiv.org/abs/1204.5406
%X We report a list of groups consisting of dwarf galaxies only. The sample
contains 126 objects, mainly combined in pairs. The most populated group
contains six dwarf galaxies. The majority of systems considered reside in the
low-density regions and evolve unaffected by massive galaxies. The
characteristic sizes and velocity dispersions of groups are 30 kpc and 11 km/s,
respectively. They resemble the associations of dwarf galaxies, but are more
compact. On the whole, groups and associations form a continuous sequence.
Alike the associations, our groups possess high mass-to-luminosity ratios, what
is indicative of a large amount of dark matter present in these systems.
@misc{makarov2012dwarf,
abstract = {We report a list of groups consisting of dwarf galaxies only. The sample
contains 126 objects, mainly combined in pairs. The most populated group
contains six dwarf galaxies. The majority of systems considered reside in the
low-density regions and evolve unaffected by massive galaxies. The
characteristic sizes and velocity dispersions of groups are 30 kpc and 11 km/s,
respectively. They resemble the associations of dwarf galaxies, but are more
compact. On the whole, groups and associations form a continuous sequence.
Alike the associations, our groups possess high mass-to-luminosity ratios, what
is indicative of a large amount of dark matter present in these systems.},
added-at = {2012-04-25T18:14:48.000+0200},
author = {Makarov, D. I. and Uklein, R. I.},
biburl = {https://www.bibsonomy.org/bibtex/2ba86839de07462034f4682929b0772fc/dolly.carrillo},
description = {[1204.5406] A List of Dwarf Galaxies in the Local Supercluster},
doi = {10.1134/S1990341312020010},
interhash = {1f40e04a40c616b1b3ff92535d8f33e6},
intrahash = {ba86839de07462034f4682929b0772fc},
keywords = {catalogue galaxy},
note = {cite arxiv:1204.5406Comment: 17 pages, 6 figures, 2 tables, to be published in Astrophysical Bulletin 67, p.123 (2012)},
timestamp = {2012-04-25T18:14:48.000+0200},
title = {A List of Dwarf Galaxies in the Local Supercluster},
url = {http://arxiv.org/abs/1204.5406},
year = 2012
}