Brightest Cluster Galaxy Alignments in Merging Clusters
Journal Article
·
· The Astrophysical Journal (Online)
- Univ. of California, Davis, CA (United States). Dept. of Physics
- Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)
The orientations of brightest cluster galaxies (BCGs) and their host clusters tend to be aligned, but the mechanism driving this is not clear. To probe the role of cluster mergers in this process, we quantify alignments of 38 BCGs in 22 clusters undergoing major mergers (up to ~1 Gyr after first pericenter). We find alignments entirely consistent with those of clusters in general. This suggests that alignments are robust against major cluster mergers. If, conversely, major cluster mergers actually help orient the BCG, such a process is acting quickly because the orientation is in place within ~1 Gyr after first pericenter.
- Research Organization:
- Lawrence Livermore National Laboratory (LLNL), Livermore, CA (United States)
- Sponsoring Organization:
- USDOE National Nuclear Security Administration (NNSA)
- Grant/Contract Number:
- AC52-07NA27344
- OSTI ID:
- 1513121
- Report Number(s):
- LLNL-JRNL--761051; 949942
- Journal Information:
- The Astrophysical Journal (Online), Journal Name: The Astrophysical Journal (Online) Journal Issue: 1 Vol. 874; ISSN 1538-4357
- Publisher:
- Institute of Physics (IOP)Copyright Statement
- Country of Publication:
- United States
- Language:
- English
Ellipticity of brightest cluster galaxies as tracer of halo orientation and weak-lensing mass bias
|
journal | November 2019 |
Merging Cluster Collaboration: A Panchromatic Atlas of Radio Relic Mergers
|
journal | September 2019 |
| Merging Cluster Collaboration: A Panchromatic Atlas of Radio Relic Mergers | text | January 2018 |
| Ellipticity of Brightest Cluster Galaxies as tracer of halo orientation and weak-lensing mass bias | text | January 2019 |
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