The interstellar dust properties of nearby galaxies
This article gives an overview of the constitution, physical conditions, and observables of
dust in the interstellar medium of nearby galaxies. We first review the macroscopic, spatial …
dust in the interstellar medium of nearby galaxies. We first review the macroscopic, spatial …
An overview of the dwarf galaxy survey
SC Madden, A Rémy-Ruyer, M Galametz… - Publications of the …, 2013 - iopscience.iop.org
ABSTRACT The Dwarf Galaxy Survey (DGS) program is studying low-metallicity galaxies
using 230 hr of far-infrared (FIR) and submillimetre (submm) photometric and spectroscopic …
using 230 hr of far-infrared (FIR) and submillimetre (submm) photometric and spectroscopic …
The star formation activity of IllustrisTNG galaxies: main sequence, UVJ diagram, quenched fractions, and systematics
M Donnari, A Pillepich, D Nelson… - Monthly Notices of …, 2019 - academic.oup.com
We select galaxies from the IllustrisTNG hydrodynamical simulations (at 0≤ z≤ 2) and
characterize the shapes and evolutions of their UVJ and star formation rate–stellar mass …
characterize the shapes and evolutions of their UVJ and star formation rate–stellar mass …
The applicability of far-infrared fine-structure lines as star formation rate tracers over wide ranges of metallicities and galaxy types
I De Looze, D Cormier, V Lebouteiller… - Astronomy & …, 2014 - aanda.org
Aims. We analyze the applicability of far-infrared fine-structure lines [Cii] 158 μm,[Oi] 63 μm,
and [Oiii] 88 μm to reliably trace the star formation rate (SFR) in a sample of low-metallicity …
and [Oiii] 88 μm to reliably trace the star formation rate (SFR) in a sample of low-metallicity …
Calibrating extinction-free star formation rate diagnostics with 33 GHz free–free emission in NGC 6946
Using free–free emission measured in the Ka band (26–40 GHz) for 10 star-forming regions
in the nearby galaxy NGC 6946, including its starbursting nucleus, we compare a number of …
in the nearby galaxy NGC 6946, including its starbursting nucleus, we compare a number of …
Efficient three-dimensional NLTE dust radiative transfer with SKIRT
We present an updated version of SKIRT, a three-dimensional (3D) Monte Carlo radiative
transfer code developed to simulate dusty galaxies. The main novel characteristics of the …
transfer code developed to simulate dusty galaxies. The main novel characteristics of the …
Herschel -ATLAS: rapid evolution of dust in galaxies over the last 5 billion years
We present the first direct and unbiased measurement of the evolution of the dust mass
function of galaxies over the past 5 billion years of cosmic history using data from the …
function of galaxies over the past 5 billion years of cosmic history using data from the …
A COOL DUST FACTORY IN THE CRAB NEBULA: A HERSCHEL* STUDY OF THE FILAMENTS
Whether supernovae are major sources of dust in galaxies is a long-standing debate. We
present infrared and submillimeter photometry and spectroscopy from the Herschel Space …
present infrared and submillimeter photometry and spectroscopy from the Herschel Space …
The Herschel Reference Survey: dust in early-type galaxies and across the Hubble Sequence
We present Herschel observations of 62 early-type galaxies (ETGs), including 39 galaxies
morphologically classified as S0+ S0a and 23 galaxies classified as ellipticals using SPIRE …
morphologically classified as S0+ S0a and 23 galaxies classified as ellipticals using SPIRE …
Revealing the cold dust in low-metallicity environments-I. Photometry analysis of the Dwarf Galaxy Survey with Herschel
Context. We present new photometric data from our Herschel guaranteed time key
programme, the Dwarf Galaxy Survey (DGS), dedicated to the observation of the gas and …
programme, the Dwarf Galaxy Survey (DGS), dedicated to the observation of the gas and …