activity
20192026
most citedThe evolution of dust in discs influenced by external photoevaporation

90 citations · 444 across the 28 of their papers we have counts for

collaborators
Showing 2024Show all

8 papers · 1 filter

astro-ph.EP2024★ 23 cited

MINDS. JWST-MIRI reveals a peculiar CO-rich chemistry in the drift-dominated disk CX Tau

Marissa Vlasblom, Milou Temmink, Sierra L. Grant +20

Radial drift of icy pebbles can have a large impact on the chemistry of the inner regions of protoplanetary disks. Compact dust disks (50 au) are suggested to have a high…

astro-ph.EP2024★ 6 cited

Hidden under a warm blanket: If planets existed in protostellar disks, they would hardly produce observable substructures

P. Nazari, A. D. Sellek, G. P. Rosotti

The onset of planet formation is actively under debate. Recent mass measurements of disks around protostars suggest an early start of planet formation in the Class 0/I disks. Howev…

astro-ph.EP2024★ 5 cited

JWST captures a sudden stellar outburst and inner disk wall destruction

Chengyan Xie, Ilaria Pascucci, Dingshan Deng +6

We present JWST/MIRI observations of T~Cha, a highly variable (3-5\,mag) accreting Sun-like star surrounded by a disk with a large (\,au) dust gap. We find that t…

astro-ph.SR2024

MINDS. JWST-MIRI Observations of a Spatially Resolved Atomic Jet and Polychromatic Molecular Wind Toward SY Cha

Kamber R. Schwarz, Matthias Samland, Göran Olofsson +21

The removal of angular momentum from protostellar systems drives accretion onto the central star and may drive the dispersal of the protoplanetary disk. Winds and jets can contribu…

astro-ph.EP2024★ 31 cited

Photoevaporation of protoplanetary discs with PLUTO+PRIZMO I. Lower X-ray-driven mass-loss rates due to enhanced cooling

Andrew D. Sellek, Tommaso Grassi, Giovanni Picogna +3

Context: Photoevaporation is an important process for protoplanetary disc dispersal but there has so far been a lack of consensus from simulations over the mass-loss rates and the…

astro-ph.EP2024★ 16 cited

Modeling JWST MIRI-MRS Observations of T Cha: Mid-IR Noble Gas Emission Tracing a Dense Disk Wind

Andrew D. Sellek, Naman S. Bajaj, Ilaria Pascucci +8

[Ne II] 12.81 emission is a well-used tracer of protoplanetary disk winds due to its blueshifted line profile. MIRI-MRS recently observed T Cha, detecting this line a…

astro-ph.EP2024

JWST MIRI/MRS Observations of T Cha: Discovery of a Spatially Resolved Disk Wind

Naman S. Bajaj, Ilaria Pascucci, Uma Gorti +8

Understanding when and how circumstellar disks disperse is crucial to constrain planet formation and migration. Thermal winds powered by high-energy stellar photons have long been…

astro-ph.EP2024

Correlation between accretion rate and free-free emission in protoplanetary disks -- A multi-wavelength analysis of central mm/cm emission in transition disks

Alessia A. Rota, Jurrian D. Meijerhof, Nienke van der Marel +3

The inner regions of protoplanetary disks are the locations where most of planets are thought to form and where processes that influence the global evolution of the disk, such as M…