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Query : 2019ApJ...875..105P |
2019ApJ...875..105P - Astrophys. J., 875, 105-105 (2019/April-3)
Do halos that form early, have high concentration, are part of a pair, or contain a central galaxy potential host more pronounced planes of satellite galaxies?
PAWLOWSKI M.S., BULLOCK J.S., KELLEY T. and FAMAEY B.
Abstract (from CDS):
Abstract Copyright: © 2019. The American Astronomical Society. All rights reserved.
Journal keyword(s): dark matter - galaxies: kinematics and dynamics - Galaxy: halo - Galaxy: structure - Local Group
Simbad objects: 5
Number of rows : 5 |
N | Identifier | Otype |
ICRS (J2000) RA |
ICRS (J2000) DEC |
Mag U | Mag B | Mag V | Mag R | Mag I | Sp type |
#ref
1850 - 2024 |
#notes |
---|---|---|---|---|---|---|---|---|---|---|---|---|
1 | NAME Andromeda XXVII | G | 00 37 27.1 | +45 23 13 | 16.7 | ~ | 75 | 0 | ||||
2 | M 31 | AGN | 00 42 44.330 | +41 16 07.50 | 4.86 | 4.36 | 3.44 | ~ | 12650 | 1 | ||
3 | NAME M 81-82 Group | GrG | 09 55 | +69.1 | ~ | 717 | 0 | |||||
4 | NAME Centaurus A | Sy2 | 13 25 27.61521044 | -43 01 08.8050291 | 8.18 | 6.84 | 6.66 | ~ | 4486 | 3 | ||
5 | NAME Local Group | GrG | ~ | ~ | ~ | 8391 | 0 |
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