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most citedNo Expanding Fireball: Resolving the Recurrent Nova RS Ophiuchi with Infrared Interferometry

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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-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…

astro-ph2005

Keck Interferometer Observations of FU Orionis Objects

R. Millan-Gabet, J. D. Monnier, R. L. Akeson +31

We present new K-band long baseline interferometer observations of three young stellar objects of the FU Orionis class, V1057 Cyg, V1515 Cyg and Z CMa-SE, obtained at the Keck Inte…

astro-ph2005

The dusty AGB star RS CrB: first mid-infrared interferometric observations with the Keck Telescopes

B. Mennesson, C. Koresko, M. J. Creech-Eakman +2

We report interferometric observations of the semi-regular variable star RS CrB, a red giant with strong silicate emission features. The data were among the first long baseline mid…

astro-ph2005

Keck Interferometer observations of classical and weak line T Tauri stars

R. L. Akeson, A. F. Boden, J. D. Monnier +9

We present observations of the T Tauri stars BP Tau, DG Tau, DI Tau, GM Aur, LkCa 15, RW Aur and V830 Tau, using long baseline infrared interferometry at K band (2.2 microns) from…

astro-ph2005

The near-infrared size-luminosity relations for Herbig Ae/Be disks

J. D. Monnier, R. Millan-Gabet, R. Billmeier +31

We report the results of a sensitive K-band survey of Herbig Ae/Be disk sizes using the 85-m baseline Keck Interferometer. Targets were chosen to span the maximum range of stellar…