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20092026
most citedDisks ARound TTauri Stars with Sphere (DARTTS-S) I: Sphere / IRDIS Polarimetric Imaging of 8 prominent TTauri Disks

365 citations · 2.9k across the 51 of their papers we have counts for

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Showing 2019Show all

7 papers · 1 filter

astro-ph.EP2019★ 63 cited

The widest H survey of accreting protoplanets around nearby transition disks

A. Zurlo, G. Cugno, M. Montesinos +6

The mechanisms of planet formation are still under debate. We know little about how planets form, even if more than 4000 exoplanets have been detected to date. Recent investigation…

astro-ph.EP2019★ 83 cited

Disks Around T Tauri Stars with SPHERE (DARTTS-S) II: Twenty-one new polarimetric images of young stellar disks

Antonio Garufi, Henning Avenhaus, Sebastian Perez +8

Near-IR polarimetric images of protoplanetary disks enable us to characterize substructures that might be due to the interaction with (forming) planets. The available census is str…

astro-ph.SR2019★ 187 cited

Kinematic detection of a planet carving a gap in a protoplanetary disc

C. Pinte, G. van der Plas, F. Menard +10

We still do not understand how planets form, or why extra-solar planetary systems are so different from our own solar system. But the last few years have dramatically changed our v…

astro-ph.EP2019★ 84 cited

Kinematic detections of protoplanets: a Doppler-flip in the disk of HD100546

Simon Casassus, Sebastian Perez

Protoplanets and circumplanetary disks are rather elusive in their thermal IR emission. Yet they are cornerstone to the most popular interpretations for the protoplanetary disks st…

astro-ph.EP2019★ 27 cited

Cooling in the shade of warped transition disks

Simon Casassus, Sebastian Perez, Axel Osses +1

The mass of the gaseous reservoir in young circumstellar disks is a crucial initial condition for the formation of planetary systems, but estimates vary by orders of magnitude. In…

astro-ph.SR2019★ 97 cited

The Ophiuchus DIsk Survey Employing ALMA (ODISEA): Disk Dust Mass Distributions across Protostellar Evolutionary Classes

Jonathan P. Williams, Lucas Cieza, Antonio Hales +5

As protostars evolve from optically faint / infrared bright (Class I) sources to optically bright / infrared faint (Class II) the solid material in their surrounding disks accumula…