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20092026
most citedHerschel Detects a Massive Dust Reservoir in Supernova 1987A

368 citations · 4k across the 100 of their papers we have counts for

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Showing 2014Show all

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astro-ph.SR2014★ 194 cited

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

M. Matsuura, E. Dwek, M. J. Barlow +33

We present new Herschel photometric and spectroscopic observations of Supernova 1987A, carried out in 2012. Our dedicated photometric measurements provide new 70 micron data and im…

astro-ph.GA2014★ 72 cited

Dust Destruction Rates and Lifetimes in the Magellanic Clouds

Tea Temim, Eli Dwek, Kirill Tchernyshyov +4

The nature, composition, abundance, and size distribution of dust in galaxies is determined by the rate at which it is created in the different stellar sources and destroyed by int…

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…

astro-ph.SR2014★ 15 cited

Principal Component Analysis of Molecular Clouds: Can CO reveal the dynamics?

Erik Bertram, Rahul Shetty, Simon C. O. Glover +3

We use Principal Component Analysis (PCA) to study the gas dynamics in numerical simulations of typical MCs. Our simulations account for the non-isothermal nature of the gas and in…