activity
20202026
most citedModeling accretion shocks at the disk-envelope interface -- Sulfur chemistry

55 citations · 119 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.SR2026

JOYS: Launch and destruction of dust in protostellar jets. The case of BHR71-IRS1 with JWST MIRI

Łukasz Tychoniec, Logan Francis, Maria Gabriela Navarro +25

Protostellar winds can theoretically lift solids from the planet-forming disks, but direct evidence for launched dust has been scarce so far. Numerous atomic lines that are unique…

astro-ph.SR2026★ 1 cited

JOYS: JWST MIRI/MRS spectra of the inner 500 au region of the L1527 IRS bipolar outflow

R. Devaraj, E. F. van Dishoeck, T. P. Ray +12

This study characterized the physical and kinematic properties within the innermost 500 au region of the L1527 bipolar outflow, a class 0/I low-mass protostar using JWST MIRI/MRS s…

astro-ph.SR2026

Characterizing the physical and chemical properties of the Class I protostellar system Oph-IRS 44. Binarity, infalling streamers, and accretion shocks

E. Artur de la Villarmois, V. V. Guzmán, M. L. van Gelder +5

(Abridged) In the low-mass star formation process, theoretical models predict that material from the infalling envelope could be shocked as it encounters the outer regions of the d…

astro-ph.GA2025★ 12 cited

JOYS: The [D/H] abundance derived from protostellar outflows across the Galactic disk measured with JWST

L. Francis, E. F. van Dishoeck, A. Caratti o Garatti +8

The total deuterium abundance [D/H] in the universe is set by just two processes: the creation of deuterium in Big Bang Nucleosynthesis at an abundance of [D/H]$=2.58\pm0.13\times1…

astro-ph.SR2021★ 55 cited

Modeling accretion shocks at the disk-envelope interface -- Sulfur chemistry

M. L. van Gelder, B. Tabone, E. F. van Dishoeck +1

As material from an infalling protostellar envelope hits the forming disk, an accretion shock may develop which could (partially) alter the envelope material entering the disk. Obs…

astro-ph.EP2020★ 51 cited

Chemically tracing the water snowline in protoplanetary disks with HCO

M. Leemker, M. L. R. van 't Hoff, L. Trapman +4

[Abridged] Planet formation is expected to be enhanced around snowlines in protoplanetary disks, in particular around the water snowline. However, the close proximity of the water…