activity
20102024
most citedFrom the Convergence of Filaments to Disk-Outflow Accretion: Massive-Star Formation in W33A

114 citations · 213 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.GA2024★ 2 cited

On the relation between magnetic field strength and gas density in the interstellar medium: A multiscale analysis

D. J. Whitworth, S. Srinivasan, R. E. Pudritz +19

The magnetic field strength to gas density relation in the interstellar medium is of fundamental importance. We present and compare Bayesian analyses of the B-n relation for two co…

astro-ph.GA2023★ 18 cited

ATOMS: ALMA Three-millimeter Observations of Massive Star-forming regions -XIII. Ongoing triggered star formation within clump-fed scenario found in the massive ( ) clump

S. Zhang, K. Wang, T. Liu +16

Whether ionization feedback triggers the formation of massive stars is highly debated. Using ALMA 3 mm observations with a spatial resolution of pc and a mass sensitivi…

astro-ph.GA2023★ 71 cited

ATOMS: ALMA Three-millimeter Observations of Massive Star-forming regions -- XV. Steady Accretion from Global Collapse to Core Feeding in Massive Hub-filament System SDC335

Feng-Wei Xu, Ke Wang, Tie Liu +37

We present ALMA Band-3/7 observations towards "the Heart" of a massive hub-filament system (HFS) SDC335, to investigate its fragmentation and accretion. At a resolution of $\sim0.0…

astro-ph.GA2022★ 8 cited

The kinetic and magnetic energy budget of hub-filament systems during the gravitational fragmentation of molecular clouds

Vianey Camacho, Enrique Vázquez-Semadeni, Manuel Zamora-Avilés +1

We present a numerical study of the balance between the gravitational (Eg), kinetic (Ek), and magnetic (Em) energies of structures within a hub-filament system in a simulation of t…

astro-ph.GA2010★ 114 cited

From the Convergence of Filaments to Disk-Outflow Accretion: Massive-Star Formation in W33A

Roberto Galván-Madrid, Qizhou Zhang, Eric Keto +5

Interferometric observations of the W33A massive star-formation region, performed with the Submillimeter Array (SMA) and the Very Large Array (VLA) at resolutions from 5 arcsec (0.…