798 citations · 3.3k across the 13 of their papers we have counts for
7 papers · 1 filter
Coagulation of small grains in disks: the influence of residual infall and initial small-grain content
C. Dominik, C. P. Dullemond
Turbulent coagulation in protoplanetary disks is known to operate on timescale far shorter than the lifetime of the disk. In the absence of mechanisms that replenish the small dust…
Flaring and self-shadowed disks around Herbig Ae stars: simulations for 10 micron interferometers
R. van Boekel, C. P. Dullemond, C. Dominik
We present simulations of the interferometric visibilities of Herbig Ae star disks. We investigate whether interferometric measurements in the 10 micrometer atmospheric window are…
Dust coagulation in protoplanetary disks: a rapid depletion of small grains
C. P. Dullemond, C. Dominik
We model the process of dust coagulation in protoplanetary disks and calculate how it affects their observational appearance. Our model involves the detailed solution of the coagul…
The effect of dust settling on the appearance of protoplanetary disks
C. P. Dullemond, C. Dominik
We analyze how the process of dust settling affects the spectral energy distribution and optical appearance of protoplanetary disks. Using simple analytic estimates on the one hand…
Flaring vs. self-shadowed disks: the SEDs of Herbig Ae/Be stars
C. P. Dullemond, C. Dominik
Isolated Herbig Ae stars can be divided into two groups (Meeus et al. 2001): those with an almost flat spectral energy distribution in the mid-infrared (`group I'), and those with…
Understanding the spectra of isolated Herbig stars in the frame of a passive disk model
C. Dominik, C. P. Dullemond, L. B. F. M. Waters +1
We discuss spectral energy distributions of a sample of Herbig Ae/Be stars in the context of a passive irradiated disk model. The data have been presented earlier by Meeus et al (2…