most citedInterferometric Observations of RS Ophiuchi and the Origin of the Near-IR Emission

15 citations · 19 across the 3 of their papers we have counts for

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astro-ph200852 cited

The limb-darkened Arcturus; Imaging with the IOTA/IONIC interferometer

S. Lacour, S. Meimon, E. Thiebaut +14

This paper is an H band interferometric examination of Arcturus, a star frequently used as a spatial and spectral calibrator. Using the IOTA 3 telescope interferometer, we performe…

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-ph200840 cited

First Images of R Aquarii and its Asymmetric HO Shell

S. Ragland, H. Le Coroller, E. Pluzhnik +7

We report imaging observations of the symbotic long-period Mira variable R Aquarii (R Aqr) at near-infrared and radio wavelengths. The near-infrared observations were made with the…

astro-ph200796 cited

Visual/infrared interferometry of Orion Trapezium stars: Preliminary dynamical orbit and aperture synthesis imaging of the Theta 1 Orionis C system

S. Kraus, Y. Y. Balega, J. -P. Berger +10

Located in the Orion Trapezium cluster, Theta 1 Orionis C is one of the youngest and nearest high-mass stars (O5-O7) and also known to be a close binary system. Using new multi-epo…

astro-ph200615 cited

Interferometric Observations of RS Ophiuchi and the Origin of the Near-IR Emission

B. F. Lane, J. L. Sokoloski, R. K. Barry +7

We report observations of the recurrent nova RS Oph using long-baseline near-IR interferometry. We are able to resolve emission from the nova for several weeks after the February 2…

astro-ph200636 cited

No Expanding Fireball: Resolving the Recurrent Nova RS Ophiuchi with Infrared Interferometry

J. D. Monnier, R. K. Barry, W. A. Traub +17

Following the recent outburst of the recurrent nova RS Oph on 2006 Feb 12, we measured its near-infrared size using the IOTA, Keck, and PTI Interferometers at multiple epochs. The…