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20012009
most citedCfA3: 185 Type Ia Supernova Light Curves from the CfA

524 citations · 1.2k across the 18 of their papers we have counts for

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22 papers · 1 filter

astro-ph20084 cited

Searching for the signatures of jet-ISM interactions in X-ray binaries

James Miller-Jones, Christian Kaiser, Tom Maccarone +8

Jets from X-ray binaries are continuously injecting matter and energy into the surrounding interstellar medium (ISM). However, there exist to date relatively few cases where jet-IS…

astro-ph200819 cited

Milliarcsecond N-Band Observations of the Nova RS Ophiuchi: First Science with the Keck Interferometer Nuller

R. K. Barry, W. C. Danchi, W. A. Traub +38

We report observations of the nova RS Ophiuchi (RS Oph) using the Keck Interferometer Nuller (KIN), approximately 3.8 days following the most recent outburst that occurred on 2006…

astro-ph200796 cited

IPHAS and the symbiotic stars. I. Selection method and first discoveries

R. L. M. Corradi, E. R. Rodríguez-Flores, A. Mampaso +7

The study of symbiotic stars is essential to understand important aspects of stellar evolution in interacting binaries. Their observed population in the Galaxy is however poorly kn…

astro-ph200764 cited

A Comparison of the Variability of the Symbiotic X-ray Binaries GX 1+4, 4U 1954+31, and 4U 1700+24 from Swift/BAT and RXTE/ASM Observations

R. H. D. Corbet, J. L. Sokoloski, K. Mukai +2

We present an analysis of the X-ray variability of three symbiotic X-ray binaries, GX 1+4, 4U 1700+24, and 4U 1954+31, using observations made with the Swift Burst Alert Telescope…

astro-ph200790 cited

An Expanding Shell and Synchrotron Jet in RS Ophiuchi

Michael P. Rupen, Amy J. Mioduszewski, Jennifer L. Sokoloski

We report high-resolution radio imaging of the recurrent nova RS Ophiuchi (RS Oph) during the first month of the 2006 outburst, using the Very Long Baseline Array (VLBA). Observati…

astro-ph20075 cited

High energy X-ray emission from recurrent novae in quiescence: T CrB

Gerardo J. M. Luna, Jennifer L. Sokoloski, Koji Mukai

We present Suzaku X-ray observations of the recurrent nova T CrB in quiescence. T CrB is the first recurrent nova to be detected in the hard-X-ray band (E ~ 40.0 keV) during quiesc…