activity
20062008
most citedThe Cassiopeia A Supernova was of Type IIB

324 citations · 967 across the 10 of their papers we have counts for

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astro-ph200846 cited

The Dust-to-Gas Ratio in the Small Magellanic Cloud Tail

K. D. Gordon, C. Bot, E. Muller +21

The Tail region of the Small Magellanic Cloud (SMC) was imaged using the MIPS instrument on the Spitzer Space Telescope as part of the SAGE-SMC Spitzer Legacy. Diffuse infrared emi…

astro-ph200858 cited

Variable Evolved Stars and YSOs Discovered in the Large Magellanic Cloud using the SAGE Survey

Uma P. Vijh, M. Meixner, B. Babler +13

We present initial results and source lists of variable sources in the Large Magellanic Cloud (LMC) for which we detect thermal infrared variability from the SAGE (Surveying the Ag…

astro-ph200818 cited

Photoevaporation of Protoplanetary Disks

Z. Balog, G. H. Rieke, J. Muzerolle +4

We present HST/NICMOS Paschen alpha images and low and high resolution IRS spectra of photoevaporating disk-tail systems originally detected at 24 micron near O stars. We find no P…

astro-ph200813 cited

The Rate and Spatial Distribution of Novae in M101 (NGC 5457)

E. A. Coelho, A. W. Shafter, K. A. Misselt

A new multi-epoch H-alpha imaging study of M101 (NGC 5457) has been carried out as part of a larger campaign to study the rate and stellar population of extragalactic novae. The su…

astro-ph2008324 cited

The Cassiopeia A Supernova was of Type IIB

Oliver Krause, Stephan M. Birkmann, Tomonori Usuda +4

Cassiopeia A is one of the youngest supernova remnants known in the Milky Way and a unique laboratory for supernova physics. We present an optical spectrum of the Cassiopeia A supe…

astro-ph2008258 cited

The Behavior of the Aromatic Features in M101 HII Regions: Evidence for Dust Processing

Karl D. Gordon, Charles W. Engelbracht, George H. Rieke +3

The aromatic features in M101 were studied spectroscopically and photometrically using observations from all three instruments on the Spitzer Space Telescope. The global SED of M10…