A list of groups of dwarf galaxies in the local supercluster

2012 ◽  
Vol 67 (2) ◽  
pp. 135-146 ◽  
Author(s):  
D. I. Makarov ◽  
R. I. Uklein
Keyword(s):  
Dwarf Galaxies ◽  
Local Supercluster

scholarly journals The Orientation of Galaxies in Nearby Galaxy Groups

2004 ◽  
Vol 217 ◽  
pp. 116-117
Author(s):  
P. Flin ◽  
M. Biernacka ◽  
J. Krywult
Keyword(s):  
Statistical Analysis ◽  
Milky Way ◽  
Random Distribution ◽  
Local Group ◽  
Dwarf Galaxies ◽  
Nearby Galaxy ◽  
Groups Of Galaxies ◽  
Galaxy Groups ◽  
Isotropic Distribution ◽  
Local Supercluster

The statistical analysis of six nearby groups of galaxies, connected with the Milky Way, M31, M81, M101, NGC5128 and NGC5236 shows an isotropic distribution of galaxy planes, similarly to galaxies within the Local Group. Also planes of galaxies in the nearby (Vr < 500 km s−1) region of the Local Supercluster exhibit random distribution, disregarding their membership to groups. The result shows that strong environmental effects observed among dwarf galaxies do not change generally random distribution of galaxy planes in this region.

A search for gas-rich dwarf galaxies just outside the Local Supercluster

1992 ◽  
Vol 104 ◽  
pp. 2086 ◽  
Author(s):  
G. L. Hoffman ◽  
Nanyao Y. Lu ◽  
E. E. Salpeter
Keyword(s):  
Dwarf Galaxies ◽  
Local Supercluster

scholarly journals Superclustering: Theory Versus Observations

1988 ◽  
Vol 130 ◽  
pp. 245-254
Author(s):  
Jaan Einasto ◽  
Maret Einasto ◽  
Enn Saar ◽  
Bernard J. T. Jones ◽  
Vicent J. Martinez
Keyword(s):  
Dark Matter ◽  
Spatial Distribution ◽  
Fractal Dimension ◽  
Galaxy Formation ◽  
Multifractal Analysis ◽  
Cold Dark Matter ◽  
Dwarf Galaxies ◽  
Local Supercluster ◽  
Theory Versus

The spatial distribution of galaxies is compared with model distributions. It is demonstrated that giant and dwarf galaxies in the Local Supercluster occupy statistically identical regions. Various tests suggest that galaxy formation is biased since all unbiased model distributions are in conflict with observed distribution of galaxies. Multifractal analysis shows that a cold dark matter dominated universe with biased galaxy formation has a fairly constant fractal dimension over a broad range of scales. This contrasts with the observed distribution which does not show simple fractal features.

scholarly journals New probable dwarf galaxies in northern groups of the Local Supercluster

2007 ◽  
Vol 33 (8) ◽  
pp. 512-519 ◽  
Author(s):  
I. D. Karachentsev ◽  
V. E. Karachentseva ◽  
W. K. Huchtmeier
Keyword(s):  
Dwarf Galaxies ◽  
Local Supercluster

scholarly journals Isolated dwarf galaxies in the local supercluster and its surroundings

Astrophysics ◽  
2010 ◽  
Vol 53 (4) ◽  
pp. 462-474 ◽  
Author(s):  
V. E. Karachentseva ◽  
I. D. Karachentsev ◽  
M. E. Sharina
Keyword(s):  
Dwarf Galaxies ◽  
Local Supercluster

scholarly journals Groups of Dwarf Galaxies in the Local Supercluster

2011 ◽  
Vol 48 ◽  
pp. 289-294 ◽  
Author(s):  
D. Makarov ◽  
I. Karachentsev ◽  
R. Uklein
Keyword(s):  
Dwarf Galaxies ◽  
Local Supercluster

scholarly journals HI-observations of dwarf galaxies in the Local Supercluster

2009 ◽  
Vol 506 (2) ◽  
pp. 677-680 ◽  
Author(s):  
W. K. Huchtmeier ◽  
I. D. Karachentsev ◽  
V. E. Karachentseva
Keyword(s):  
Dwarf Galaxies ◽  
Local Supercluster
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