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20072026
most citedA Magnetized Jet from a Massive Protostar

198 citations · 1.9k across the 55 of their papers we have counts for

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24 papers · 1 filter

astro-ph.SR2025★ 7 cited

Detailed Microwave Continuum Spectra from Bright Protoplanetary Disks in Taurus

Caleb Painter, Sean M. Andrews, Claire J. Chandler +9

We present new observations that densely sample the microwave (4-360 GHz) continuum spectra from eight young systems in the Taurus region. Multi-component, empirical model prescrip…

astro-ph.SR2023

An SiO Toroid and Wide-angle Outflow associated with the Massive Protostar W75N(B)-VLA2

Jose F. Gomez, Jose M. Torrelles, Josep M. Girart +12

We have carried out ALMA observations of the massive star-forming region W75N(B), which contains the massive protostars VLA1, VLA2, and VLA3. Particularly, VLA2 is an enigmatic pro…

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.SR2023★ 24 cited

Forbidden emission lines in protostellar outflows and jets with MUSE

Lizxandra Flores-Rivera, Mario Flock, Nicolás Kurtovic +14

Forbidden emission lines in protoplanetary disks are a key diagnostic in studies of the evolution of the disk and the host star. We report spatially resolved emission lines, [OI] 6…

astro-ph.SR2021★ 22 cited

Zooming into the Collimation Zone in a Massive Protostellar Jet

Carlos Carrasco-González, Alberto Sanna, Adriana Rodríguez-Kamenetzky +5

Protostellar jets have a fundamental role at the earliest evolution of protostars of all masses. In the case of low-mass (<8 Msun) protostars, strong observational evidence exists…

astro-ph.SR2019★ 30 cited

Modeling the accretion disk around the high-mass protostar GGD 27-MM1

N. Añez-Lopez, M. Osorio, G. Busquet +9

Recent high-angular resolution (40 mas) ALMA observations at 1.14 mm resolve a compact (R~200 au) flattened dust structure perpendicular to the HH 80-81 jet emanating from the GGD…