372 citations · 6.9k across the 115 of their papers we have counts for
116 papers
Filament Formation via Collision-induced Magnetic Reconnection -- Kinematic Features
Shuo Kong, Griselda Arroyo-Chávez, Volker Ossenkopf-Okada +4
The Collision-induced Magnetic Reconnection (CMR) mechanism has recently been proposed as a filament formation model that emphasizes the active role of magnetic fields. To enable b…
PROJECT-J: JWST observations of HH46~IRS and its outflow. Overview and first results
B. Nisini, M. G. Navarro, T. Giannini +23
We present the first results of the JWST program PROJECT-J (PROtostellar JEts Cradle Tested with JWST ), designed to study the Class I source HH46 IRS and its outflow through NIRSp…
The ALMA Legacy survey of Class 0/I disks in Corona australis, Aquila, chaMaeleon, oPhiuchus north, Ophiuchus, Serpens (CAMPOS). I. Evolution of Protostellar disk radii
Cheng-Han Hsieh, Héctor G. Arce, María José Maureira +5
We surveyed nearly all the embedded protostars in seven nearby clouds (Corona Australis, Aquila, Chamaeleon I & II, Ophiuchus North, Ophiuchus, Serpens) with the Atacama Large Mill…
On the magnetic field properties of protostellar envelopes in Orion
Bo Huang, Josep M. Girart, Ian W. Stephens +23
We present 870 um polarimetric observations toward 61 protostars in the Orion molecular clouds, with ~400 au (1") resolution using the Atacama Large Millimeter/submillimeter Array.…
CMR exploration II -- filament identification with machine learning
Duo Xu, Shuo Kong, Avichal Kaul +2
We adopt magnetohydrodynamics (MHD) simulations that model the formation of filamentary molecular clouds via the collision-induced magnetic reconnection (CMR) mechanism under varyi…
Binary Formation in a 100 m-dark Massive Core
Shuo Kong, Héctor G. Arce, John J. Tobin +4
We report high-resolution ALMA observations toward a massive protostellar core C1-Sa (30 M) in the Dragon Infrared Dark Cloud. At the resolution of 140 AU, the core f…