most citedScale-dependent surface and volume density properties of filaments in molecular clouds

1 citations · 1 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.GA2026

ALMA-IMF XXII. Role of core subfragmentation in the IMF origin: Hierarchical fragmentation cascade and CMF in W43-MM1

F. Motte, N. Le Nestour, R. Veyry +29

We aim to predict how the currently observed top-heavy CMF in the massive protocluster W43-MM1 evolves due to core subfragmentation. We used getsf to extract sources in 5 ALMA imag…

astro-ph.GA2026

A Salpeter-like filament linear density function across nearby molecular clouds

Guo-Yin Zhang, Alexander Men'shchikov, Jin-Zeng Li

The high-mass slope of the stellar initial mass function (IMF), first measured by Salpeter in 1955, appears nearly universal across star-forming environments, yet its physical orig…

astro-ph.GA2026

Deriving volume density profiles of filaments from observed surface densities

Alexander Men'shchikov, Guo-Yin Zhang

Accurate characterization of filamentary structures in star-forming clouds is essential for understanding star formation. Traditional methods fit observed surface density profiles…

astro-ph.GA20261 cited

Scale-dependent surface and volume density properties of filaments in molecular clouds

Guo-Yin Zhang, Alexander Men'shchikov, Jin-Zeng Li

We present a systematic analysis of scale-dependent properties of filamentary structures in seven nearby molecular clouds Taurus, Ophiuchus, Perseus, Orion A, California, IC 51…

astro-ph.GA2026

Dense cores and filaments in M16: Enhanced formation efficiency in the stellar feedback-driven shell

Nageen Pervaiz, Guo-Yin Zhang, Alexander Men'shchikov +1

We present a comprehensive analysis of dense cores and filamentary structures in the M16 Eagle Nebula using high-resolution () surface density and temperature…