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20042017
most citedCrystalline silicates and dust processing in the protoplanetary disks of the Taurus young cluster

159 citations · 887 across the 9 of their papers we have counts for

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6 papers · 1 filter

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-ph2007★ 159 cited

Crystalline silicates and dust processing in the protoplanetary disks of the Taurus young cluster

Dan M. Watson, Jarron M. Leisenring, Elise Furlan +15

We characterize the crystalline silicate content and spatial distribution of small dust grains in a large sample of protoplanetary disks in the Taurus-Auriga young cluster, using S…

astro-ph2006★ 118 cited

Mid-Infrared Spectroscopy of Disks around Classical T Tauri Stars

W. J. Forrest, B. Sargent, E. Furlan +18

We present the first Spitzer Infrared Spectrograph (IRS; The IRS was a collaborative venture between Cornell University and Ball Aerospace Corporation funded by NASA through the Je…

astro-ph2006★ 81 cited

Dust Processing in Disks around T Tauri Stars

B. Sargent, W. J. Forrest, P. D'Alessio +11

The 8-14 micron emission spectra of 12 T Tauri stars in the Taurus/Auriga dark clouds and in the TW Hydrae association obtained with the Infrared Spectrograph (IRS; The IRS is a co…

astro-ph2006★ 79 cited

Spitzer-IRS Observations of FU Orionis Objects

J. D. Green, L. Hartmann, N. Calvet +5

We present 5-35 m spectra, taken with the Infrared Spectrograph (IRS) on the Spitzer Space Telescope, of five FU Orionis objects: FU Ori, V1515 Cyg, V1057 Cyg, BBW 76, and V346…

astro-ph2004★ 99 cited

The state of protoplanetary material 10 Myr after stellar formation: circumstellar disks in the TW Hydrae association

K. I. Uchida, N. Calvet, L. Hartmann +17

We have used the Spitzer Infrared Spectrograph to observe seven members of the TW Hya association, the nearest stellar association whose age ( 10 Myr) is similar to the times…