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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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Posted ContentDOI

The physical connection between central stellar surface density and stellar spin in SAMI and MaNGA nearby galaxies

TL;DR: In this article , the stellar surface density within the inner 1 kpc (Σ1) has become a popular tool for understanding the growth of galaxies and its connection with the quenching of star formation.
Journal ArticleDOI

A stochastic model to reproduce the star-formation history of individual galaxies in hydrodynamic simulations

TL;DR: In this paper , a model to describe individual galaxies' star formation history (SFH) from three simulations is presented, which divides the galaxy SFH into two distinct components: the main sequence and the variance.
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No Evolution in the Half-mass Radius of Milky Way–type Galaxies over the Last 10 Gyr

TL;DR: In this article , the stellar-mass growth history (SMGH) of the Milky Way (MW) galaxy is studied, and it is shown that the progenitors of the MW galaxy grow self-similarly on spatially resolved scales with roughly a constant half-mass radius (∼2-3 kpc) over the past 10 Gyr, while their stellar masses increase by about 1 dex.
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.
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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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