Massive Quenched Galaxies at z ∼ 0.7 Retain Large Molecular Gas Reservoirs

Massive Quenched Galaxies at z ∼ 0.7 Retain Large Molecular Gas Reservoirs

The physical mechanisms that quench star formation, turning blue star-forming galaxies into red quiescent galaxies, remain unclear. In this Letter, we investigate the role of gas supply in suppressing star formation by studying the molecular gas content of post-starburst galaxies. Leveraging the wid...

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Bibliographic Details
Main Authors: Suess, Katherine A., Bezanson, Rachel, Spilker, Justin S., Kriek, Mariska, Greene, Jenny E., Feldmann, Robert, Hunt, Qiana, Narayanan, Desika
Other Authors: Univ Arizona, Steward Observ
Language:en
Published: IOP PUBLISHING LTD 2017
Subjects:
galaxies: evolution
galaxies: formation
Online Access:http://hdl.handle.net/10150/625739
http://arizona.openrepository.com/arizona/handle/10150/625739

Internet

http://hdl.handle.net/10150/625739
http://arizona.openrepository.com/arizona/handle/10150/625739

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