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The growth of the central region by acquisition of counterrotating gas in star-forming galaxies

Chen, Yan-Mei; Shi, Yong; Tremonti, Christy A.; Bershady, Matt; Merrifield, Michael; Emsellem, Eric; Jin, Yi-Fei; Huang, Song; Fu, Hai; Wake, David A.; Bundy, Kevin; Stark, David; Lin, Lihwai; Argudo-Fernandez, Maria; Bergmann, Thaisa Storchi; Bizyaev, Dmitry; Brownstein, Joel; Bureau, Martin; Chisholm, John; Drory, Niv; Guo, Qi; Hao, Lei; Hu, Jian; Li, Cheng; Li, Ran; Lopes, Alexandre Roman; Pan, Kai-Ke; Riffel, Rogemar A.; Thomas, Daniel; Wang, Lan; Westfall, Kyle; Yan, Ren-Bin

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Authors

Yan-Mei Chen

Yong Shi

Christy A. Tremonti

Matt Bershady

Michael Merrifield

Eric Emsellem

Yi-Fei Jin

Song Huang

Hai Fu

David A. Wake

Kevin Bundy

David Stark

Lihwai Lin

Maria Argudo-Fernandez

Thaisa Storchi Bergmann

Dmitry Bizyaev

Joel Brownstein

Martin Bureau

John Chisholm

Niv Drory

Qi Guo

Lei Hao

Jian Hu

Cheng Li

Ran Li

Alexandre Roman Lopes

Kai-Ke Pan

Rogemar A. Riffel

Daniel Thomas

Lan Wang

Kyle Westfall

Ren-Bin Yan



Abstract

Galaxies grow through both internal and external processes. In about 10% of nearby red galaxies with little star formation, gas and stars are counter-rotating, demonstrating the importance of external gas acquisition in these galaxies. However, systematic studies of such phenomena in blue, star-forming galaxies are rare, leaving uncertain the role of external gas acquisition in driving evolution of blue galaxies. Here, based on new measurements with integral field spectroscopy of a large representative galaxy sample, we find an appreciable fraction of counter-rotators among blue galaxies (9 out of 489 galaxies). The central regions of blue counter-rotators show younger stellar populations and more intense, ongoing star formation than their outer parts, indicating ongoing growth of the central regions. The result offers observational evidence that the acquisition of external gas in blue galaxies is possible; the interaction with pre-existing gas funnels the gas into nuclear regions (<1 kpc) to form new stars.

Citation

Chen, Y.-M., Shi, Y., Tremonti, C. A., Bershady, M., Merrifield, M., Emsellem, E., Jin, Y.-F., Huang, S., Fu, H., Wake, D. A., Bundy, K., Stark, D., Lin, L., Argudo-Fernandez, M., Bergmann, T. S., Bizyaev, D., Brownstein, J., Bureau, M., Chisholm, J., Drory, N., …Yan, R.-B. (2016). The growth of the central region by acquisition of counterrotating gas in star-forming galaxies. Nature Communications, 7, Article 13269. https://doi.org/10.1038/ncomms13269

Journal Article Type Article
Acceptance Date Sep 16, 2016
Online Publication Date Oct 19, 2016
Publication Date 2016-12
Deposit Date Oct 20, 2016
Publicly Available Date Oct 20, 2016
Journal Nature Communications
Electronic ISSN 2041-1723
Publisher Nature Publishing Group
Peer Reviewed Peer Reviewed
Volume 7
Article Number 13269
DOI https://doi.org/10.1038/ncomms13269
Public URL https://nottingham-repository.worktribe.com/output/822520
Publisher URL http://www.nature.com/articles/ncomms13269
Contract Date Oct 20, 2016

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