activity
20192025
most citedALMA observations and modeling of the rotating outflow in Orion Source I

11 citations · 34 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2025★ 2 cited

The Rotation Dip in the Envelope-Disk Transition of HH 111: Evidence for Magnetic Braking

Jyun-Heng Lin, Chin-Fei Lee, Zhi-Yun Li +3

Magnetic braking can drive angular momentum loss in star formation and influence disk evolution. A previous study of HH 111 VLA1 suggested a decrease in rotation velocity in a regi…

astro-ph.SR2024★ 10 cited

ALMA Survey of Orion Planck Galactic Cold Clumps (ALMASOP): Nested Morphological and Kinematic Structures of Outflows Revealed in SiO and CO Emission

Chun-Fan Liu, Hsien Shang, Doug Johnstone +22

The Atacama Large Millimeter/submillimeter Array Survey of Orion Planck Galactic Cold Clumps (ALMASOP) reveals complex nested morphological and kinematic features of molecular outf…

astro-ph.SR2023★ 1 cited

Multiple shells driven by disk winds: ALMA observations in the HH 30 outflow

J. A. López-Vázquez, Chin-Fei Lee, M. Fernández-López +3

We present archive Atacama Large Millimeter/Submillimeter Array (ALMA) Band 6 observations of the CO (J=2-1) and CO (J=2-1) molecular line emission of the protostella…

astro-ph.GA2023★ 1 cited

Episodic Accretion in Protostars -- An ALMA Survey of Molecular Jets in the Orion Molecular Cloud

Somnath Dutta, Chin-Fei Lee, Doug Johnstone +20

Protostellar outflows and jets are almost ubiquitous characteristics during the mass accretion phase, and encode the history of stellar accretion, complex-organic molecule (COM) fo…

astro-ph.SR2020★ 11 cited

ALMA observations and modeling of the rotating outflow in Orion Source I

J. A. López-Vázquez, Luis A. Zapata, Susana Lizano +1

We present SiO(J=8--7) =0, SiS (J=19--18) =0, and SiO (J=8--7) =1 molecular line archive observations made with the Atacama Large Millimeter/Submillimeter Ar…

astro-ph.SR2019★ 9 cited

Angular momentum in bipolar outflows: dynamical evolutionary model

J. A. López-Vázquez, J. Cantó, S. Lizano

We model molecular outflows produced by the time dependent interaction between a stellar wind and a rotating cloud envelope in gravitational collapse, studied by Ulrich. We conside…