C
Cornelis P. Dullemond
Researcher at Heidelberg University
Publications - 351
Citations - 32120
Cornelis P. Dullemond is an academic researcher from Heidelberg University. The author has contributed to research in topics: Accretion (astrophysics) & Radiative transfer. The author has an hindex of 98, co-authored 344 publications receiving 29106 citations. Previous affiliations of Cornelis P. Dullemond include University of Amsterdam & Maine Principals' Association.
Papers
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Journal ArticleDOI
The Disk Substructures at High Angular Resolution Project (DSHARP). I. Motivation, Sample, Calibration, and Overview
Sean M. Andrews,Jane Huang,Laura M. Pérez,Andrea Isella,Cornelis P. Dullemond,Nicolás T. Kurtovic,Viviana V. Guzmán,John M. Carpenter,David J. Wilner,Shangjia Zhang,Zhaohuan Zhu,Tilman Birnstiel,Xue-Ning Bai,Myriam Benisty,Myriam Benisty,A. Meredith Hughes,Karin I. Öberg,Luca Ricci +17 more
TL;DR: The Disk Substructures at High Angular Resolution Project (DSHARP) as mentioned in this paper was the first large-scale project to find and characterize substructures in the spatial distributions of solid particles for a sample of 20 nearby protoplanetary disks, using very high resolution (similar to 0'' 035 or 5 au, FWHM) observations of their 240 GHz (1.25 mm) continuum emission.
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Passive Irradiated Circumstellar Disks with an Inner Hole
TL;DR: In this article, a model for irradiated dust disks around Herbig Ae stars is proposed, based on the flaring disk model given by Chiang and Goldreich in 1997, but with the central regions of the disk removed.
Journal ArticleDOI
Resolved Images of Large Cavities in Protoplanetary Transition Disks
Sean M. Andrews,David J. Wilner,Catherine Espaillat,Annie Hughes,Cornelis P. Dullemond,Melissa McClure,Chunhua Qi,Joanna M. Brown +7 more
TL;DR: In this article, the authors present new and archival high angular resolution (03 40-75 AU) Submillimeter Array (SMA) observations of the 880 μm (340 GHz) dust continuum emission from 12 transition disks in nearby star-forming regions.
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Coagulation, fragmentation and radial motion of solid particles in protoplanetary disks
TL;DR: In this article, the authors presented the results of numerical simulations with more and more realistic physics involved, including various effects, such as particle growth, radial/vertical particle motion and dust particle fragmentation in their simulations.
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Protoplanetary disk structures in ophiuchus
TL;DR: In this paper, the authors presented the results of a high angular resolution (0.3 -40 AU) survey of the 345 GHz (870 -mu) thermal continuum emission from nine of the brightest, and therefore most massive, circumstellar disks in the Ophiuchus star-forming region.