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20042026
most citedA Survey and Analysis of Spitzer Infrared Spectrograph Spectra of T Tauri Stars in Taurus

411 citations · 3.2k across the 43 of their papers we have counts for

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astro-ph2008★ 96 cited

Silica in Protoplanetary Disks

B. A. Sargent, W. J. Forrest, C. Tayrien +10

Mid-infrared spectra of a few T Tauri stars (TTS) taken with the Infrared Spectrograph (IRS) on board the Spitzer Space Telescope show prominent narrow emission features indicating…

astro-ph2008★ 44 cited

A slowly accreting ~10 Myr old transitional disk in Orion OB1a

C. Espaillat, J. Muzerolle, J. Hernandez +7

Here we present the Spitzer IRS spectrum of CVSO 224, the sole transitional disk located within the ~10 Myr old 25 Orionis group in Orion OB1a. A model fit to the spectral energy d…

astro-ph2008★ 144 cited

Epsilon Eridani's Planetary Debris Disk: Structure and Dynamics based on Spitzer and CSO Observations

D. Backman, M. Marengo, K. Stapelfeldt +9

Spitzer and Caltech Submillimeter Observatory (CSO) images and spectrophotometry of epsilon Eridani at wavelengths from 3.5 to 350 um reveal new details of its bright debris disk.…

astro-ph2007★ 288 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…

astro-ph2007★ 70 cited

The Dust and Gas Around beta Pictoris

C. H. Chen, A. Li, C. Bohac +12

We have obtained Spitzer IRS 5.5 - 35 micron spectroscopy of the debris disk around beta Pictoris. In addition to the 10 micron silicate emission feature originally observed from t…

astro-ph2006★ 411 cited

A Survey and Analysis of Spitzer Infrared Spectrograph Spectra of T Tauri Stars in Taurus

E. Furlan, L. Hartmann, N. Calvet +9

We present mid-infrared spectra of T Tauri stars in the Taurus star-forming region obtained with the Spitzer Infrared Spectrograph (IRS). For the first time, the 5-36 micron spectr…