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Revealing the relation between black-hole growth and host-galaxy compactness among star-forming galaxies
- Publication Year :
- 2020
-
Abstract
- Recent studies show that a universal relation between black-hole (BH) growth and stellar mass ($M_\bigstar$) or star formation rate (SFR) is an oversimplification of BH-galaxy co-evolution, and that morphological and structural properties of host galaxies must also be considered. Particularly, a possible connection between BH growth and host-galaxy compactness was identified among star-forming (SF) galaxies. Utilizing $\approx 6300$ massive galaxies with $I_{\rm 814W}~<br />Comment: 21 pages, 21 figures. Accepted for publication in MNRAS
- Subjects :
- Physics
Stellar mass
010308 nuclear & particles physics
Star formation
Star (game theory)
FOS: Physical sciences
Velocity dispersion
Sigma
Astronomy and Astrophysics
Astrophysics
Astrophysics::Cosmology and Extragalactic Astrophysics
01 natural sciences
Astrophysics - Astrophysics of Galaxies
Galaxy
Space and Planetary Science
Astrophysics of Galaxies (astro-ph.GA)
0103 physical sciences
Content (measure theory)
Astrophysics::Earth and Planetary Astrophysics
Connection (algebraic framework)
010303 astronomy & astrophysics
Astrophysics::Galaxy Astrophysics
Subjects
Details
- Language :
- English
- Database :
- OpenAIRE
- Accession number :
- edsair.doi.dedup.....a3a1c5fe4a1628cd7f26b7a31d90ef4c