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most citedDust Properties of Protoplanetary Disks in the Taurus-Auriga Star Forming Region from Millimeter Wavelengths

403 citations · 2.8k across the 25 of their papers we have counts for

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6 papers · 1 filter

astro-ph2006★ 115 cited

Accretion in protoplanetary disks: the imprint of core properties

C. P. Dullemond, A. Natta, L. Testi

In this Letter we present a theoretical scenario to explain the steep correlation between disk accretion rates and stellar masses observed in pre-main sequence stars. We show that…

astro-ph2003★ 18 cited

An analysis of two-layer models for circumstellar disks

C. P. Dullemond, A. Natta

The two-layer disk models of Chiang & Goldreich (1997, henceforth CG) and its derivatives are popular among astronomers because of their simplicity and the clear predictions they m…

astro-ph2002★ 172 cited

Vertical structure models of T Tauri and Herbig Ae/Be disks

C. P. Dullemond, G. J. van Zadelhoff, A. Natta

In this paper we present detailed models of the vertical structure (temperature and density) of passive irradiated circumstellar disks around T Tauri and Herbig Ae/Be stars. In con…

astro-ph2001★ 215 cited

H2 and CO emission from disks around TTauri and HerbigAe pre-main-sequence stars and from debris disks around young stars: warm and cold circumstellar gas

W. F. Thi, E. F. van Dishoeck, G. A. Blake +8

We present ISO-SWS observations of H2 pure-rotational line emission from the disks around low and intermediate mass pre-main-sequence stars as well as from young stars thought to b…

astro-ph2001★ 82 cited

NICS-TNG low-resolution 0.85-2.45um spectra of L-Dwarfs: a near-infrared spectral classification scheme for faint dwarfs

L. Testi, F. D'Antona, F. Ghinassi +8

We present complete near-infrared (0.85-2.45 um), low-resolution (~100) spectra of a sample of 26 disk L-dwarfs with reliable optical spectral type classification. The observations…

astro-ph2001★ 89 cited

Constraints on properties of the protoplanetary disks around UX Ori and CQ Tau

L. Testi, A. Natta, D. S. Shepherd +1

We present Very Large Array observations of the intermediate mass pre-main-sequence stars UX Ori and CQ Tau at 7mm, 3.6cm, and 6cm. These stars are members of the UX Ori variabilit…