Yun Hsin Hsu
SDSS-IV MaNGA: Cannibalism Caught in the Act - On the Frequency of Occurrence of Multiple Cores in Brightest Cluster Galaxies
Hsu, Yun Hsin; Lin, Yen Ting; Huang, Song; Nelson, Dylan; Rodriguez-Gomez, Vicente; Lai, Hsuan Ting; Greene, Jenny; Leauthaud, Alexie; Aragón-Salamanca, Alfonso; Bundy, Kevin; Emsellem, Eric; Merrifield, Michael; More, Surhud; Okabe, Nobuhiro; Rong, Yu; Brownstein, Joel R.; Lane, Richard R.; Pan, Kaike; Schneider, Donald P.
Authors
Yen Ting Lin
Song Huang
Dylan Nelson
Vicente Rodriguez-Gomez
Hsuan Ting Lai
Jenny Greene
Alexie Leauthaud
Professor ALFONSO ARAGON-SALAMANCA ALFONSO.ARAGON@NOTTINGHAM.AC.UK
Professor of Astronomy
Kevin Bundy
Eric Emsellem
Michael Merrifield
Surhud More
Nobuhiro Okabe
Yu Rong
Joel R. Brownstein
Richard R. Lane
Kaike Pan
Donald P. Schneider
Abstract
Although it is generally accepted that massive galaxies form in a two-phased fashion, beginning with a rapid mass buildup through intense starburst activities followed by primarily dry mergers that mainly deposit stellar mass at outskirts, the late time stellar mass growth of brightest cluster galaxies (BCGs), the most massive galaxies in the universe, is still not well understood. Several independent measurements have indicated a slower mass growth rate than predictions from theoretical models. We attempt to resolve the discrepancy by measuring the frequency of BCGs with multiple cores, which serve as a proxy of the merger rates in the central region and facilitate a more direct comparison with theoretical predictions. Using 79 BCGs at z = 0.06-0.15 with integral field spectroscopic data from the Mapping Nearby Galaxies at Apache Point Observatory (MaNGA) project, we obtain a multiple-core fraction of 0.11 ± 0.04 at z ≈ 0.1 within an 18 kpc radius from the center, which is comparable to the value of 0.08 ± 0.04 derived from mock observations of 218 simulated BCGs from the cosmological hydrodynamical simulation IllustrisTNG. We find that most cores that appear close to the BCGs from imaging data turn out to be physically associated systems. Anchoring on the similarity in the multiple-core frequency between the MaNGA and IllustrisTNG, we discuss the mass growth rate of BCGs over the past 4.5 Gyr.
Citation
Hsu, Y. H., Lin, Y. T., Huang, S., Nelson, D., Rodriguez-Gomez, V., Lai, H. T., …Schneider, D. P. (2022). SDSS-IV MaNGA: Cannibalism Caught in the Act - On the Frequency of Occurrence of Multiple Cores in Brightest Cluster Galaxies. Astrophysical Journal, 933(1), Article 61. https://doi.org/10.3847/1538-4357/ac6d66
Journal Article Type | Article |
---|---|
Acceptance Date | May 3, 2022 |
Online Publication Date | Jul 4, 2022 |
Publication Date | Jul 1, 2022 |
Deposit Date | May 12, 2022 |
Publicly Available Date | May 12, 2022 |
Journal | Astrophysical Journal |
Print ISSN | 0004-637X |
Electronic ISSN | 1538-4357 |
Publisher | American Astronomical Society |
Peer Reviewed | Peer Reviewed |
Volume | 933 |
Issue | 1 |
Article Number | 61 |
DOI | https://doi.org/10.3847/1538-4357/ac6d66 |
Keywords | Space and Planetary Science; Astronomy and Astrophysics |
Public URL | https://nottingham-repository.worktribe.com/output/8046374 |
Publisher URL | https://iopscience.iop.org/article/10.3847/1538-4357/ac6d66 |
Additional Information | Article Title: SDSS-IV MaNGA: Cannibalism Caught in the Act—On the Frequency of Occurrence of Multiple Cores in Brightest Cluster Galaxies; Journal Title: The Astrophysical Journal; Article Type: paper; Copyright Information: © 2022. The Author(s). Published by the American Astronomical Society.; Date Received: 2021-12-19; Date Accepted: 2022-05-03; Online publication date: 2022-07-04 |
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Publisher Licence URL
https://creativecommons.org/licenses/by/4.0/
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