most citedA stubbornly large mass of cold dust in the ejecta of Supernova 1987A

194 citations · 620 across the 5 of their papers we have counts for

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astro-ph.GA2015★ 48 cited

Star-formation rates from young-star counts and the structure of the ISM across the NGC346/N66 complex in the SMC

S. Hony, D. A. Gouliermis, F. Galliano +21

The rate at which interstellar gas is converted into stars, and its dependence on environment, is one of the pillars on which our understanding of the visible Universe is build. We…

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★ 70 cited

The influence of supernova remnants on the interstellar medium in the Large Magellanic Cloud seen at 20--600 m wavelengths

Maša Lakićević, Jacco Th. van Loon, Margaret Meixner +20

We present the analysis of supernova remnants (SNRs) in the Large Magellanic Cloud (LMC) and their influence on the environment at far-infrared (FIR) and submillimeter wavelengths.…

astro-ph.GA2014★ 176 cited

Dust and Gas in the Magellanic Clouds from the HERITAGE Herschel Key Project. I. Dust Properties and Insights into the Origin of the Submm Excess Emission

Karl D. Gordon, Julia Roman-Duval, Caroline Bot +33

The dust properties in the Large and Small Magellanic Clouds are studied using the HERITAGE Herschel Key Project photometric data in five bands from 100 to 500 micron. Three simple…