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20172021
most citedGravity Driven Magnetic Field at ~1000 au Scales in High-mass Star Formation

100 citations · 249 across the 7 of their papers we have counts for

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12 papers · 1 filter

astro-ph.GA2021100 cited

Gravity Driven Magnetic Field at ~1000 au Scales in High-mass Star Formation

Patricio Sanhueza, Josep Miquel Girart, Marco Padovani +20

A full understanding of high-mass star formation requires the study of one of the most elusive components of the energy balance in the interstellar medium: magnetic fields. We repo…

astro-ph.GA202139 cited

Digging into the Interior of Hot Cores with ALMA (DIHCA). I. Dissecting the High-mass Star-Forming Core G335.579-0.292 MM1

Fernando A. Olguin, Patricio Sanhueza, Andrés E. Guzmán +10

We observed the high-mass star-forming region G335.579-0.292 with the Atacama Large Millimeter/submillimeter Array (ALMA) at 226 GHz with an angular resolution of 0.3'' ($\sim 1000…

astro-ph.GA2020

SiO emission as a probe of Cloud-Cloud Collisions in Infrared Dark Clouds

G. Cosentino, I. Jiménez-Serra, J. D. Henshaw +6

Infrared Dark Clouds (IRDCs) are very dense and highly extincted regions that host the initial conditions of star and stellar cluster formation. It is crucial to study the kinemati…

astro-ph.GA20208 cited

Cloud structures in M17 SWex : Possible cloud-cloud collision

Shinichi W. Kinoshita, Fumitaka Nakamura, Quang Nguyen-Luong +11

Using wide-field CO () data taken with the Nobeyama 45-m telescope, we investigate cloud structures of the infrared dark cloud complex in M17 with SCIMES. In total, w…

astro-ph.GA2019

GMC Collisions as Triggers of Star Formation. VII. The Effect of Magnetic Field Strength on Star Formation

Benjamin Wu, Jonathan C. Tan, Duncan Christie +1

We investigate the formation of stars within giant molecular clouds (GMCs) evolving in environments of different global magnetic field strength and large-scale dynamics. Building u…

astro-ph.GA2019

The ALMA Survey of 70 m dark High-mass clumps in Early Stages (ASHES). I. Pilot Survey: Clump Fragmentation

Patricio Sanhueza, Yanett Contreras, Benjamin Wu +20

(Abridged) ASHES has been designed to systematically characterize the earliest stages and to constrain theories of high-mass star formation. A total of 12 massive (>500