activity
20032008
most citedProplyds and Massive Disks in the Orion Nebula Cluster Imaged with CARMA and SMA

98 citations · 353 across the 6 of their papers we have counts for

collaborators

10 papers

astro-ph200898 cited

Proplyds and Massive Disks in the Orion Nebula Cluster Imaged with CARMA and SMA

J. A. Eisner, R. L. Plambeck, John M. Carpenter +3

[Abridged] We imaged a 2' x 2' region of the Orion Nebula cluster in 1.3 mm wavelength continuum emission with the recently commissioned Combined Array for Research in Millimeter A…

astro-ph200713 cited

Interferometric Observations of V1663 Aquilae (Nova Aql 2005)

B. F. Lane, A. Retter, J. A. Eisner +3

We have resolved the classical nova V1663 Aql using long-baseline near-IR interferometry covering the period from 5--18 days after peak brightness. We directly measure the shape an…

astro-ph200761 cited

Water vapour and hydrogen in the terrestrial-planet-forming region of a protoplanetary disk

J. A. Eisner

Planetary systems, ours included, are formed in disks of dust and gas around young stars. Disks are an integral part of the star and planet formation process, and knowledge of the…

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-ph200668 cited

Spectrally Dispersed K-Band Interferometric Observations of Herbig Ae/Be Sources: Inner Disk Temperature Profiles

J. A. Eisner, E. I. Chiang, B. F. Lane +1

We use spectrally dispersed near-IR interferometry data to constrain the temperature profiles of sub-AU-sized regions of 11 Herbig Ae/Be sources. We find that a single-temperature…

astro-ph2006

Spatially Resolving the Inner Disk of TW Hya

J. A. Eisner, E. I. Chiang, L. A. Hillenbrand

We present Keck Interferometer observations of TW Hya that spatially resolve its emission at 2 micron wavelength. Analyzing these data together with existing K-band veiling and nea…