activity
20152026
most citedConsistent dust and gas models for protoplanetary disks. I. Disk shape, dust settling, opacities, and PAHs

379 citations · 1.4k across the 35 of their papers we have counts for

collaborators
Showing 2023Show all

5 papers · 1 filter

astro-ph.EP2023★ 11 cited

Disk Evolution Study Through Imaging of Nearby Young Stars (DESTINYS): HD 34700 A unveils an inner ring

G. Columba, E. Rigliaco, R. Gratton +18

Context. The study of protoplanetary disks is fundamental to understand their evolution and interaction with the surrounding environment, and to constrain planet formation mechanis…

astro-ph.EP2023★ 25 cited

Hydrocarbon chemistry in inner regions of planet forming disks

Jayatee Kanwar, Inga Kamp, Peter Woitke +3

The analysis of the mid-infrared spectra helps understanding the composition of the gas in the inner, dense and warm terrestrial planet forming region of disks around young stars.…

astro-ph.EP2023★ 22 cited

Constraining the gas distribution in the PDS 70 disk as a method to assess the effect of planet-disk interactions

B. Portilla-Revelo, I. Kamp, S. Facchini +7

Embedded planets are potentially the cause of substructures like gaps and cavities observed in several protoplanetary disks. Thus, the substructures observed in the continuum and i…

astro-ph.SR2023★ 11 cited

Disk Evolution Study Through Imaging of Nearby Young Stars (DESTINYS): Diverse outcomes of binary-disk interactions

Yapeng Zhang, Christian Ginski, Jane Huang +15

Circumstellar disks do not evolve in isolation, as about half of solar-type stars were born in binary or multiple systems. Resolving disks in binary systems provides the opportunit…

astro-ph.SR2023★ 8 cited

Massive pre-main-sequence stars in M17 -- Modelling hydrogen and dust in MYSO disks

Frank Backs, J. Poorta, Ch. Rab +5

The young massive-star-forming region M17 contains optically visible massive pre-main-sequence stars that are surrounded by circumstellar disks. Such disks are expected to disappea…