Alma Observations of Massive Molecular Gas Filaments Encasing Radio Bubbles in the Phoenix Cluster

Alma Observations of Massive Molecular Gas Filaments Encasing Radio Bubbles in the Phoenix Cluster

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We report new ALMA observations of the CO(3-2) line emission from the 2.1 +/- 0.3*10(10)M(circle dot). molecular gas reservoir in the central galaxy of the Phoenix cluster. The cold molecular gas is fueling a vigorous starburst at a rate of 500-800M(circle dot)yr(-1) and powerful black hole activity...

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Bibliographic Details
Main Authors: Russell, H. R., McDonald, M., McNamara, B. R., Fabian, A. C., Nulsen, P. E. J., Bayliss, M. B., Benson, B. A., Brodwin, M., Carlstrom, J. E., Edge, A. C., Hlavacek-Larrondo, J., Marrone, D. P., Reichardt, C. L., Vieira, J. D.
Other Authors: Univ Arizona, Steward Observ
Language:en
Published: IOP PUBLISHING LTD 2017
Subjects:
galaxies: active
galaxies: clusters
individual (Phoenix)
radio lines: galaxies
Online Access:http://hdl.handle.net/10150/623241
http://arizona.openrepository.com/arizona/handle/10150/623241

Internet

http://hdl.handle.net/10150/623241
http://arizona.openrepository.com/arizona/handle/10150/623241

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