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19992008
most citedOn the Diversity of the Taurus Transitional Disks: UX Tau A & Lk Ca 15

288 citations · 1.3k across the 17 of their papers we have counts for

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astro-ph200855 cited

Long-wavelength excesses of FU Orionis objects: flared outer disks or infalling envelopes?

Zhaohuan Zhu, Lee Hartmann, Nuria Calvet +3

The mid- to far-infrared emission of the outbursting FU Orionis objects has been attributed either to a flared outer disk or to an infalling envelope. We revisit this issue using d…

astro-ph200888 cited

Constraining the Envelope Structure of L1527 IRS: Infrared Scattered Light Modeling

John J. Tobin, Lee Hartmann, Nuria Calvet +1

We model Spitzer Space Telescope observations of the Taurus Class 0 protostar L1527 IRS (IRAS 04368+2557) to provide constraints on its protostellar envelope structure. The nearly…

astro-ph20081 cited

Spitzer IRS Observations of Disks around Brown Dwarfs in the TW Hydra Association

A. L. Morrow, K. L. Luhman, C. Espaillat +8

Using SpeX at the NASA Infrared Telescope Facility and the Spitzer Infrared Spectrograph, we have obtained infrared spectra from 0.7 to 30um for three young brown dwarfs in the TW…

astro-ph200815 cited

A sub-AU outwardly truncated accretion disk around a classical T Tauri star

M. K. McClure, W. J. Forrest, B. A. Sargent +10

We present the Spitzer Infrared Spectrograph (IRS) spectrum of SR20, a 5--10 AU binary T Tauri system in the Ophiuchi star forming region. The spectrum has features consistent…

astro-ph2007120 cited

Spitzer IRS Spectra and Envelope Models of Class I Protostars in Taurus

E. Furlan, M. McClure, N. Calvet +8

We present Spitzer Infrared Spectrograph spectra of 28 Class I protostars in the Taurus star-forming region. The 5 to 36 micron spectra reveal excess emission from the inner region…

astro-ph2007288 cited

On the Diversity of the Taurus Transitional Disks: UX Tau A & Lk Ca 15

C. Espaillat, N. Calvet, P. D'Alessio +5

The recently recognized class of "transitional disk" systems consists of young starswith optically-thick outer disks but inner disks which are mostly devoid of small dust. Here we…