most citedDense Molecular Clumps with Large Blue Asymmetries: Evidence for Collapse

2 citations · 2 across the 4 of their papers we have counts for

collaborators

5 papers

astro-ph.GA2026

Global and Local Infall in the ASHES Sample (GLASHES). III. Physical Parameters of Contracting Motion onto Dense Cores in 70 m Dark Massive Clumps

Kaho Morii, Patricio Sanhueza, Qizhou Zhang +3

Core growth is a key process in high-mass star formation. As part of the GLASHES (Global and Local Infall in the ASHES Sample) survey, we present infall velocities and mass infall…

astro-ph.GA2026

Molecular cloud dispersal traced by the ionized carbon 158 micron line

L. Bonne, N. Schneider, S. Dannhauer +14

Feedback from massive stars in the form of radiation and winds impacts the associated host molecular cloud. Feedback can disperse cloud material and lead to the destruction of the…

astro-ph.GA2026

Global and Local Infall in the ASHES Sample (GLASHES). II. Asymmetric Line Profiles around Dense Cores in 70 m Dark Massive Clumps

Kaho Morii, Patricio Sanhueza, Qizhou Zhang +1

Gravitational collapse is fundamental to star formation, yet direct kinematic evidence of infall at the core scale in high-mass star-forming regions remains poorly constrained. We…

astro-ph.GA2026★ 2 cited

Dense Molecular Clumps with Large Blue Asymmetries: Evidence for Collapse

James M. Jackson, J. Scott Whitaker, Edward Chambers +10

An analysis of the Millimetre Astronomy Legacy Team 90 GHz (MALT90) survey has produced a sample of 27 candidate dense molecular clumps with large collapse motions, as revealed by…

astro-ph.GA2025

Magnetic Fields in the Bones of the Milky Way

Ian W. Stephens, Simon Coude, Philip C. Myers +20

Stars primarily form in galactic spiral arms within dense, filamentary molecular clouds. The largest and most elongated of these molecular clouds are referred to as ``bones," which…