activity
20072020
most citedClouds, filaments and protostars: the Herschel Hi-GAL Milky Way

806 citations · 2.6k across the 15 of their papers we have counts for

collaborators

15 papers

astro-ph.GA2020★ 65 cited

Powderday: Dust Radiative Transfer for Galaxy Simulations

Desika Narayanan, Matthew J. Turk, Thomas Robitaille +18

We present Powderday, a flexible, fast, open-source dust radiative transfer package designed to interface with galaxy formation simulations. Powderday builds on FSPS population syn…

astro-ph.GA2016★ 26 cited

Earliest phases of star formation (EPoS): Dust temperature distributions in isolated starless cores

N. Lippok, R. Launhardt, Th. Henning +9

Constraining the temperature and density structure of dense molecular cloud cores is fundamental for understanding the initial conditions of star formation. We use Herschel observa…

astro-ph.GA2015★ 195 cited

The Formation of Submillimetre-Bright Galaxies from Gas Infall over a Billion Years

Desika Narayanan, Matthew Turk, Robert Feldmann +7

Submillimetre-luminous galaxies at high-redshift are the most luminous, heavily star-forming galaxies in the Universe, and are characterised by prodigious emission in the far-infra…

astro-ph.GA2014★ 132 cited

Dust and Gas in the Magellanic Clouds from the HERITAGE Herschel Key Project. II. Gas-to-Dust Ratio Variations across ISM Phases

Julia Roman-Duval, Karl Gordon, Margaret Meixner +32

The spatial variations of the gas-to-dust ratio (GDR) provide constraints on the chemical evolution and lifecycle of dust in galaxies. We examine the relation between dust and gas…

astro-ph.SR2012★ 49 cited

The standard model of low-mass star formation applied to massive stars: a multi-wavelength picture of AFGL 2591

K. G. Johnston, D. S. Shepherd, T. P. Robitaille +1

This paper aims to investigate the hypothesis that the embedded luminous star AFGL2591-VLA3 (2.3E5Lsun at 3.33kpc) is forming according to a scaled-up version of a low-mass star fo…

astro-ph.GA2012★ 70 cited

Early-stage young stellar objects in the Small Magellanic Cloud

J. M. Oliveira, J. Th. van Loon, G. C. Sloan +12

We present new observations of 34 YSO candidates in the SMC. The anchor of the analysis is a set of Spitzer-IRS spectra, supplemented by groundbased 3-5 micron spectra, Spitzer and…