Did the Milky Way Dwarf Satellites Enter The Halo as a Group?
- Author(s)
- Manuel Metz, Pavel Kroupa, Christian Theis, Gerhard Hensler
- Abstract
The dwarf satellite galaxies in the Local Group are generally considered to be hosted in dark matter subhalos that survived the disruptive processes during infall onto their host halos. It has recently been argued that if the majority of satellites entered the Milky Way (MW) halo in a group rather than individually, this could explain the spatial and dynamical peculiarities of its satellite distribution. Such groups were identified as dwarf galaxy associations that are found in the nearby universe. In this paper, we address the question whether galaxies in such associations can be the progenitors of the MW satellite galaxies. We find that the dwarf associations are much more extended than would be required to explain the disklike distribution of the MW and Andromeda satellite galaxies. We further identify a possible minor filamentary structure, perpendicular to the supergalactic plane, in which the dwarf associations are located, that might be related to the direction of infall of a progenitor galaxy of the MW satellites, if they are of tidal origin.
- Organisation(s)
- Department of Astrophysics
- External organisation(s)
- Rheinische Friedrich-Wilhelms-Universität Bonn
- Journal
- The Astrophysical Journal: an international review of astronomy and astronomical physics
- Volume
- 697
- Pages
- 269-274
- No. of pages
- 6
- ISSN
- 0004-637X
- DOI
- https://doi.org/10.1088/0004-637X/697/1/269
- Publication date
- 2009
- Peer reviewed
- Yes
- Austrian Fields of Science 2012
- 103004 Astrophysics
- Portal url
- https://ucrisportal.univie.ac.at/en/publications/948c721e-ef45-44ca-9c8c-e598b2c5adf1