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20042009
most citedImaging the Surface of Altair

331 citations · 1.2k across the 8 of their papers we have counts for

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astro-ph2008123 cited

A Tale of Two Herbig Ae stars -MWC275 and AB Aurigae: Comprehensive Models for SED and Interferometry

A. Tannirkulam, J. D. Monnier, T. J. Harries +12

We present comprehensive models for the Herbig Ae stars MWC275 and AB Aur that aim to explain their spectral energy distribution (from UV to millimeter) and long baseline interfero…

astro-ph2008271 cited

First Resolved Images of the Eclipsing and Interacting Binary Beta Lyrae

M. Zhao, D. Gies, J. D. Monnier +12

We present the first resolved images of the eclipsing binary Beta Lyrae, obtained with the CHARA Array interferometer and the MIRC combiner in the H band. The images clearly show t…

astro-ph200883 cited

Strong Near-Infrared Emission Interior to the Dust-Sublimation Radius of Young Stellar Objects MWC275 and AB Aur

A. Tannirkulam, J. D. Monnier, R. Millan-Gabet +7

Using the longest optical-interferometeric baselines currently available, we have detected strong near-infrared (NIR) emission from inside the dust-destruction radius of Herbig Ae…

astro-ph2007331 cited

Imaging the Surface of Altair

John D. Monnier, M. Zhao, E. Pedretti +13

Spatially resolving the surfaces of nearby stars promises to advance our knowledge of stellar physics. Using optical long-baseline interferometry, we present here a near-infrared i…

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-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…