PDRs4All: A JWST early release science program on radiative feedback from massive stars

PI Team, O Berné, É Habart, E Peeters… - Publications of the …, 2022 - iopscience.iop.org
The James Webb Space Telescope (JWST, Gardner et al. 2006) is a 6.5 m space telescope
launched in 2021 December and is developed by the National Aeronautics and Space …

The alma spectroscopic survey in the hubble ultra deep field: co excitation and atomic carbon in star-forming galaxies at z= 1–3

LA Boogaard, P van der Werf, A Weiss… - The Astrophysical …, 2020 - iopscience.iop.org
We investigate the CO excitation and interstellar medium (ISM) conditions in a cold gas
mass-selected sample of 22 star-forming galaxies at z= 0.46–3.60, observed as part of the …

Synthetic observations of star formation and the interstellar medium

TJ Haworth, SCO Glover, CM Koepferl, TG Bisbas… - New Astronomy …, 2018 - Elsevier
Synthetic observations are playing an increasingly important role across astrophysics, both
for interpreting real observations and also for making meaningful predictions from models. In …

A Herschel/PACS far-infrared line emission survey of local luminous infrared galaxies

T Díaz-Santos, L Armus, V Charmandaris… - The Astrophysical …, 2017 - iopscience.iop.org
We present an analysis of [] Oi 63,[Oiii] 88,[Nii] 122, and [] Cii 158 far-infrared (FIR) fine-
structure line observations obtained with Herschel/PACS, for∼ 240 local luminous infrared …

The properties of the interstellar medium of galaxies across time as traced by the neutral atomic carbon [C i]

F Valentino, GE Magdis, E Daddi, D Liu… - The Astrophysical …, 2020 - iopscience.iop.org
The Properties of the Interstellar Medium of Galaxies across Time as Traced by the Neutral
Atomic Carbon [C i] - IOPscience This site uses cookies. By continuing to use this site you …

The dust mass in Cassiopeia A from a spatially resolved Herschel analysis

I De Looze, MJ Barlow, BM Swinyard… - Monthly Notices of …, 2016 - academic.oup.com
Theoretical models predict that core-collapse supernovae (CCSNe) can be efficient dust
producers (0.1-1.0 M⊙), potentially accounting for most of the dust production in the early …

The photodissociation region toolbox: software and models for astrophysical analysis

MW Pound, MG Wolfire - The Astronomical Journal, 2022 - iopscience.iop.org
Abstract The PhotoDissociation Region Toolbox provides comprehensive, easy-to-use,
public software tools and models that enable an understanding of the interaction of the light …

Expanding bubbles in Orion A:[C ii] observations of M 42, M 43, and NGC 1977

CHM Pabst, JR Goicoechea, D Teyssier… - Astronomy & …, 2020 - aanda.org
Context. The Orion Molecular Cloud is the nearest massive-star forming region. Massive
stars have profound effects on their environment due to their strong radiation fields and …

SHINING, a survey of far-infrared lines in nearby galaxies. II. Line-deficit models, AGN impact,[C II]–SFR scaling relations, and mass–metallicity relation in (U) LIRGs

R Herrera-Camus, E Sturm… - The Astrophysical …, 2018 - iopscience.iop.org
The SHINING survey offers a great opportunity to study the properties of the ionized and
neutral media of galaxies from prototypical starbursts and active galactic nuclei (AGNs) to …

Bright extragalactic ALMA redshift survey (BEARS) III: detailed study of emission lines from 71 Herschel targets

M Hagimoto, T Bakx, S Serjeant… - Monthly Notices of …, 2023 - academic.oup.com
We analyse the molecular and atomic emission lines of 71 bright Herschel-selected galaxies
between redshifts 1.4 and 4.6 detected by the Atacama Large Millimeter/submillimeter Array …