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ALMA andHerschelreveal that X-ray-selected AGN and main-sequence galaxies have different star formation rate distributions
- Source :
- Monthly notices of the Royal Astronomical Society : letters, 2015, Vol.453(1), pp.L83-L87 [Peer Reviewed Journal]
- Publication Year :
- 2015
- Publisher :
- Oxford University Press (OUP), 2015.
-
Abstract
- Using deep Herschel and ALMA observations, we investigate the star formation rate (SFR) distributions of X-ray selected AGN host galaxies at 0.5<br />Comment: 5 pages, 3 figures, 1 table; Accepted for publication in MNRAS Letters after moderate changes
- Subjects :
- Physics
Active galactic nucleus
010308 nuclear & particles physics
Star formation
Astrophysics::High Energy Astrophysical Phenomena
FOS: Physical sciences
Astronomy
Astronomy and Astrophysics
Astrophysics::Cosmology and Extragalactic Astrophysics
Astrophysics
Astrophysics - Astrophysics of Galaxies
01 natural sciences
Galaxy
Redshift
Space and Planetary Science
Astrophysics of Galaxies (astro-ph.GA)
0103 physical sciences
Log-normal distribution
Astrophysics::Solar and Stellar Astrophysics
Astrophysics::Earth and Planetary Astrophysics
010303 astronomy & astrophysics
Astrophysics::Galaxy Astrophysics
Subjects
Details
- ISSN :
- 17453933 and 17453925
- Volume :
- 453
- Database :
- OpenAIRE
- Journal :
- Monthly Notices of the Royal Astronomical Society: Letters
- Accession number :
- edsair.doi.dedup.....bb8f7996d9bef49589408a7e67bab296