Skip to main content

Research Repository

Advanced Search

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.

SDSS-IV MaNGA: Cannibalism Caught in the Act - On the Frequency of Occurrence of Multiple Cores in Brightest Cluster Galaxies Thumbnail


Authors

Yun Hsin Hsu

Yen Ting Lin

Song Huang

Dylan Nelson

Vicente Rodriguez-Gomez

Hsuan Ting Lai

Jenny Greene

Alexie Leauthaud

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

Files





You might also like



Downloadable Citations