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
Citations
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Star formation quenching imprinted on the internal structure of naked red nuggets
Ignacio Martín-Navarro,Ignacio Martín-Navarro,Glenn van de Ven,Glenn van de Ven,Akın Yıldırım +4 more
TL;DR: In this paper, the authors investigate the spatially resolved star formation histories of a sample of 12 naked red nuggets and measure how their radial light distributions, star formation rates and central densities evolved in time.
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Must Star-forming Galaxies Rapidly Get Denser before They Quench?
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The Properties of Massive Star-forming galaxies with Outside-in Assembly Mode
TL;DR: In this article, a sample of 77 massive star-forming galaxies with an outside-in assembly mode (called targeted sample) was selected from the Mapping Nearby Galaxies at the Apache Point Observatory (MaNGA) survey.
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Baryon cycles in the biggest galaxies
Megan Donahue,G. Mark Voit +1 more
TL;DR: In this article , the authors explore the consequences of a model in which energy released during blackhole accretion shuts down star formation when sigma-v exceeds a critical value determined by the galaxy's supernova heating rate.
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The Dearth of Differences between Central and Satellite Galaxies. II. Comparison of Observations with L-GALAXIES and EAGLE in Star Formation Quenching
Enci Wang,Huiyuan Wang,Houjun Mo,Houjun Mo,Frank C. van den Bosch,S. H. Lim,Lixin Wang,Xiaohu Yang,Sihan Chen +8 more
TL;DR: The authors showed that the quenched fractions of central and satellite galaxies as a function of halo mass are extremely similar, as long as one controls for stellar and halo masses.
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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TL;DR: In this paper, the authors examined the properties of the host galaxies of 22 623 narrow-line active galactic nuclei (AGN) with 0.02 < z < 0.3 selected from a complete sample of 122 808 galaxies from the Sloan Digital Sky Survey.
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