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most citedMassive-Star Supernovae as Major Dust Factories

202 citations · 684 across the 12 of their papers we have counts for

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6 papers · 1 filter

astro-ph2007★ 172 cited

The James Clerk Maxwell Telescope Legacy Survey of Nearby Star-forming Regions in the Gould Belt

D. Ward-Thompson, J. Di Francesco, J. Hatchell +59

This paper describes a James Clerk Maxwell Telescope (JCMT) legacy survey that has been awarded roughly 500 hrs of observing time to be carried out from 2007 to 2009. In this surve…

astro-ph2006★ 27 cited

The JCMT Spectral Legacy Survey

R. Plume, G. A. Fuller, F. Helmich +30

Stars form in the densest, coldest, most quiescent regions of molecular clouds. Molecules provide the only probes which can reveal the dynamics, physics, chemistry and evolution of…

astro-ph2006★ 202 cited

Massive-Star Supernovae as Major Dust Factories

Ben E. K. Sugerman, Barbara Ercolano, M. J. Barlow +15

We present late-time optical and mid-infrared observations of the Type-II supernova 2003gd in NGC 628. Mid-infrared excesses consistent with cooling dust in the ejecta are observed…

astro-ph2005★ 42 cited

Detection of a massive dust shell around the Type II supernova SN 2002hh

M. J. Barlow, B. E. K. Sugerman, J. Fabbri +11

Dust emission from the Type II supernova SN 2002hh in NGC 6946 has been detected at mid-infrared wavelengths by the Spitzer Space Telescope from 590 to 758 days after outburst and…

astro-ph2004★ 40 cited

PAHs and crystalline silicates in the post-AGB star IRAS 16279-4757

M. Matsuura, A. A. Zijlstra, F. J. Molster +7

IRAS 16279-4757 belongs to a group of post-AGB stars showing both PAH bands and crystalline silicates. We present mid-infrared images, that resolve the object for the first time. T…

astro-ph2001★ 57 cited

Temperature effects on the 15-85-micron spectra of olivines and pyroxenes

J. E. Bowey, C. Lee, C. Tucker +3

Far-infrared spectra of laboratory silicates are normally obtained at room temperature even though the grains responsible for astronomical silicate emission bands seen at wavelengt…