activity
20052009
most citedImaging the Surface of Altair

331 citations · 949 across the 12 of their papers we have counts for

collaborators

20 papers

astro-ph.SR2009

The Formation and Evolution of Planetary Systems: The Search for and Characterization of Young Planets

Charles Beichman, Isabelle Baraffe, Christopher Crockett +16

Despite the revolution in our knowledge resulting from the detection of planets around mature stars, we know almost nothing about planets orbiting young stars because rapid rotatio…

astro-ph.SR2009

How and When do Planets Form? The Inner Regions of Planet Forming Disks at High Spatial and Spectral Resolution

R. Millan-Gabet, John D. Monnier

The formation of planets is one of the major unsolved problems in modern astrophysics. Planets are believed to form out of the material in circumstellar disks known to exist around…

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-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-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-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…