activity
20192026
most citedA statistical analysis of dust polarization properties in ALMA observations of Class 0 protostellar cores

42 citations · 146 across the 7 of their papers we have counts for

collaborators

8 papers

astro-ph.GA2026

JOYS+ analyses of OCN, NO, NO, and complex cyanides in ices -- Thermal processing results in modest enhancement of OCN ice

P. Nazari, N. Brunken, Y. Chen +12

Nitrogen-bearing molecules are more difficult to observe than oxygen-bearing ones, mainly due to the lower abundance of nitrogen in the interstellar medium. Therefore, the formatio…

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

JOYS: A JWST/MIRI survey of the evolution of H winds and jets from low-mass protostars

L. Francis, Ł. Tychoniec, E. F. van Dishoeck +20

Protostellar outflows display wide-angle winds and collimated jets, the magnetocentrifugal launching of which enables accretion onto the protostar. The majority of the outflow mass…

astro-ph.GA2024★ 6 cited

A Tale of Three: Magnetic Fields along the Orion Integral-Shaped Filament as Revealed by JCMT BISTRO survey

Jintai Wu, Keping Qiu, Frederick Poidevin +152

As part of the BISTRO survey, we present JCMT 850 m polarimetric observations towards the Orion Integral-Shaped Filament (ISF) that covers three portions known as OMC-1, OMC-2,…

astro-ph.SR2023★ 36 cited

Modest dust settling in the IRAS04302+2247 Class I protoplanetary disk

M. Villenave, L. Podio, G. Duchene +11

We present new VLA observations, between 6.8mm and 66mm, of the edge-on Class~I disk IRAS04302+2247. Observations at 6.8mm and 9.2mm lead to the detection of thermal emission from…

astro-ph.GA2020★ 42 cited

A statistical analysis of dust polarization properties in ALMA observations of Class 0 protostellar cores

V. J. M. Le Gouellec, A. J. Maury, V. Guillet +8

Recent observational progress has challenged the dust grain-alignment theories used to explain the polarized dust emission routinely observed in star-forming cores. In an effort to…

astro-ph.SR2019★ 42 cited

Understanding the origin of the magnetic field morphology in the wide-binary protostellar system BHR 71

Charles L. H. Hull, Valentin J. M. Le Gouellec, Josep M. Girart +2

We present 1.3 mm ALMA observations of polarized dust emission toward the wide-binary protostellar system BHR 71 IRS1 and IRS2. IRS1 features what appears to be a natal, hourglass-…

astro-ph.GA2019★ 20 cited

The seven most massive clumps in W43-Main as seen by ALMA: Dynamical equilibrium and Magnetic Fields

Paulo C. Cortes, Charles L. H. Hull, Josep M. Girart +8

Here we present new ALMA observations of polarized dust emission from six of the most massive clumps in W43-Main. The clumps MM2, MM3, MM4, MM6, MM7, and MM8, have been resolved in…