Decoupled black hole accretion and quenching: the relationship between BHAR, SFR and quenching in Milky Way- and Andromeda-mass progenitors since z = 2.5

Decoupled black hole accretion and quenching: the relationship between BHAR, SFR and quenching in Milky Way- and Andromeda-mass progenitors since z = 2.5

We investigate the relationship between the black hole accretion rate (BHAR) and star formation rate (SFR) for Milky Way (MW) and Andromeda (M31)-mass progenitors from z = 0.2 to 2.5. We source galaxies from the K-s-band-selected ZFOURGE survey, which includes multiwavelength data spanning 0.3-160 m...

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Bibliographic Details
Main Authors: Cowley, M. J., Spitler, L. R., Quadri, R. F., Goulding, A. D., Papovich, C., Tran, K. V. H., Labbé, I., Alcorn, L., Allen, R. J., Forrest, B., Glazebrook, K., Kacprzak, G. G., Morrison, G., Nanayakkara, T., Straatman, C. M. S., Tomczak, A. R.
Other Authors: Univ Arizona, LBT Observ
Language:en
Published: OXFORD UNIV PRESS 2018
Subjects:
galaxies: active
galaxies: evolution
galaxies: high-redshift
infrared: galaxies
Online Access:http://hdl.handle.net/10150/627058
http://arizona.openrepository.com/arizona/handle/10150/627058

Internet

http://hdl.handle.net/10150/627058
http://arizona.openrepository.com/arizona/handle/10150/627058

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