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Open AccessJournal ArticleDOI

Structural and Star-forming Relations since z similar to 3: Connecting Compact Star-forming and Quiescent Galaxies

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.

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Journal ArticleDOI

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.
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Hosts and triggers of AGNs in the Local Universe

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.
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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.
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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.
References
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Journal ArticleDOI

Stellar population synthesis at the resolution of 2003

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.
Journal ArticleDOI

Galactic stellar and substellar initial mass function

TL;DR: A review of the present-day mass function and initial mass function in various components of the Galaxy (disk, spheroid, young, and globular clusters) and in conditions characteristic of early star formation is presented in this paper.
Journal ArticleDOI

Star formation in galaxies along the hubble sequence

TL;DR: In this article, the authors focus on the broad patterns in the star formation properties of galaxies along the Hubble sequence and their implications for understanding galaxy evolution and the physical processes that drive the evolution.
Journal ArticleDOI

The Dust Content and Opacity of Actively Star-Forming Galaxies

TL;DR: In this article, far-infrared (FIR) photometry at 150 and 205 micron(s) of eight low-redshift starburst galaxies obtained with the Infrared Space Observatory (ISO) ISOPHOT is presented.
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