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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

Evidence for ram-pressure stripping in a cluster of galaxies at z = 0.7

TL;DR: In this paper, multi-unit Spectroscopic Explorer (MUSE) observations of the cluster of galaxies CGr32 at z = 0.73 reveal the presence of two massive star-forming galaxies with extended tails of diffuse gas detected in the [O'II]λλ3727−3729 A emission-line doublet.
Journal ArticleDOI

Evidence for ram pressure stripping in a cluster of galaxies at z=0.7

TL;DR: In this article, the authors show that two massive star forming galaxies with extended tails of diffuse gas detected in the [OII]$\lambda\lambda$3727-3729 A emission-line doublet.
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On the Evolution of the Central Density of Quiescent Galaxies

TL;DR: In this paper, the authors investigated the origin of the evolution of the population-averaged central stellar mass density of quiescent galaxies by probing the relation between stellar age and the zeropoint of the ridgeline down with time.
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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