Structural and Star-forming Relations since z similar to 3: Connecting Compact Star-forming and Quiescent Galaxies
Guillermo Barro,Guillermo Barro,S. M. Faber,David C. Koo,Avishai Dekel,Jerome J. Fang,Jonathan R. Trump,Pablo G. Pérez-González,Camilla Pacifici,Joel R. Primack,Rachel S. Somerville,Haojing Yan,Yicheng Guo,F. S. Liu,Daniel Ceverino,Dale D. Kocevski,Elizabeth J. McGrath +16 more
TLDR
In this article, the authors study the evolution of scaling relations that compare the effective density (Sigma(e), r 9.6 -9.3M(circle dot) kpc(-2), allowing the most efficient identification of compact SFGs and quiescent galaxies at every redshift.Abstract:
We study the evolution of the scaling relations that compare the effective density (Sigma(e), r 9.6 -9.3M(circle dot) kpc(-2), allowing the most efficient identification of compact SFGs and quiescent galaxies at every redshift.read more
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Molecular gas in distant brightest cluster galaxies
TL;DR: The stellar mass assembly of the brightest cluster galaxies (BCGs) is still debated as discussed by the authors, and the authors have observed in CO with the IRAM-30m two star forming BCGs belonging to SpARCS clusters, 3C 244.1 and SDSS J161112.5.
Journal ArticleDOI
Hosts and triggers of AGNs in the Local Universe
Ziwen Zhang,Huiyuan Wang,Wentao Luo,Wentao Luo,Houjun Mo,Zhixiong Liang,Ran Li,Xiaohu Yang,Tinggui Wang,Hong-Xin Zhang,Hui Hong,Xiaoyu Wang,Enci Wang,Pengfei Li,JingJing Shi +14 more
TL;DR: In this article, the authors compare active galactic nuclei (AGNs) with control star-forming and quiescent galaxies on galactic, inter-halo and larger scales, and find that AGNs are preferentially found in two specific stages of galaxy evolution: starburst and green valley phases.
Journal ArticleDOI
Effect of the environment on star formation activity and stellar mass for star-forming galaxies in the COSMOS field
TL;DR: In this article, the authors investigated the relationship between the environment and the galaxy main sequence (the relationship between stellar mass and star formation rate), as well as the relationship of the environment to radio luminosity, and found that the slope of the main sequence for different z and M* bins is shallower than the main-sequence consensus, with a gradual evolution towards higher redshift bins.
Journal ArticleDOI
The (Black Hole Mass)–(Spheroid Stellar Density) Relations: M <sub>BH</sub>–μ (and M <sub>BH</sub>–Σ) and M <sub>BH</sub>–ρ
TL;DR: In this article , the authors investigated the correlations between the BH mass and the projected luminosity density, the projected stellar mass density, and the deprojected internal mass density for various spheroid radii.
Journal ArticleDOI
Formation of compact galaxies in the Extreme-Horizon simulation
Solène Chabanier,Solène Chabanier,Frédéric Bournaud,Frédéric Bournaud,Yohan Dubois,Sandrine Codis,Sandrine Codis,Damien Chapon,David Elbaz,Christophe Pichon,Christophe Pichon,Olivier Bressand,Julien Devriendt,Raphael Gavazzi,Katarina Kraljic,Taysun Kimm,Clotilde Laigle,Jean-Baptiste Lekien,Garreth Martin,Garreth Martin,Nathalie Palanque-Delabrouille,Sebastien Peirani,Pierre-Franck Piserchia,Adrianne Slyz,Maxime Trebitsch,Maxime Trebitsch,Christophe Yèche +26 more
TL;DR: The Extreme-Horizon (EH) cosmological simulation as mentioned in this paper models galaxy formation with stellar and AGN feedback and uses a very high resolution in the intergalactic and circumgalactic medium.
References
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Stellar population synthesis at the resolution of 2003
Gustavo Bruzual,Stephane Charlot +1 more
TL;DR: In this article, the spectral evolution of stellar populations at ages between 100,000 yr and 20 Gyr at a resolution of 3 A across the whole wavelength range from 3200 to 9500 A for a wide range of metallicities.
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Daniela Calzetti,Lee Armus,Ralph C. Bohlin,Anne L. Kinney,J. Koornneef,Thaisa Storchi-Bergmann +5 more
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