activity
20092023
most citedGas-to-Dust mass ratios in local galaxies over a 2 dex metallicity range

661 citations · 12.2k across the 124 of their papers we have counts for

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Showing 2014Show all

14 papers · 1 filter

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.GA2014★ 115 cited

Dust continuum emission as a tracer of gas mass in galaxies

Brent A. Groves, Eva Schinnerer, Adam Leroy +8

We use a sample of 36 galaxies from the KINGFISH (Herschel IR), HERACLES (IRAM CO), and THINGS (VLA HI) surveys to study empirical relations between Herschel infrared (IR) luminosi…

astro-ph.GA2014★ 16 cited

Quantifying the Heating Sources for Mid-infrared Dust Emissions in Galaxies: The Case of M 81

Nanyao Lu, G. J. Bendo, A. Boselli +12

With the newly available SPIRE images at 250 and 500 micron from Herschel Space Observatory, we study quantitative correlations over a sub-kpc scale among three distinct emission c…

astro-ph.GA2014★ 197 cited

[CII] 158 m Emission as a Star Formation Tracer

R. Herrera-Camus, A. D. Bolatto, M. G. Wolfire +23

The [CII] 157.74 m transition is the dominant coolant of the neutral interstellar gas, and has great potential as a star formation rate (SFR) tracer. Using the Herschel KINGFISH…

astro-ph.GA2014★ 73 cited

Cool dust heating and temperature mixing in nearby star-forming galaxies

L. K. Hunt, B. T. Draine, S. Bianchi +20

Physical conditions of the interstellar medium in galaxies are closely linked to the ambient radiation field and the heating of dust grains. In order to characterize dust propertie…

astro-ph.GA2014★ 312 cited

Evolution of the dust emission of massive galaxies up to z=4 and constraints on their dominant mode of star formation

Matthieu Béthermin, Emanuele Daddi, Georgios Magdis +17

We aim to measure the average dust and molecular gas content of massive star-forming galaxies () up to z=4 in the COSMOS field to determine if the…