activity
20032025
most citedFrom filamentary clouds to prestellar cores to the stellar IMF: Initial highlights from the Herschel Gould Belt survey

1.5k citations · 6.2k across the 52 of their papers we have counts for

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Showing astro-ph.GAShow all

40 papers · 1 filter

astro-ph.GA2025★ 2 cited

ALMAGAL VII. Cataloging Hierarchical Mass Structure from Cores to Clumps across the Galactic Disk

Jennifer Wallace, Taevis Kolz, Cara Battersby +42

Investigating the multi-scale fragmentation of dense clumps into compact cores is essential for understanding the processes that govern the initial distribution of mass in stellar…

astro-ph.GA2025★ 5 cited

The Rosetta Stone Project. II. The correlation between star formation efficiency and L/M indicator for the evolutionary stages of star-forming clumps in post-processed radiative magnetohydrodynamics simulations

Ngo-Duy Tung, Alessio Traficante, Ugo Lebreuilly +13

Context. The evolution of massive star-forming clumps that are progenitors of high-mass young stellar objects are often classified based on a variety of observational indicators ra…

astro-ph.GA2025

PRIMAGAL: a PRIMAger Galactic Plane Far-IR polarization survey to quantify the magnetic fields' role in the formation and evolution of large star-forming filaments

S. Molinari, J. D. Soler, V. -M. Pelkonen +8

The PRIMAger instrument on board the proposed PRIMA satellite will offer the unprecedented capability to obtain hundreds of square-degree maps in polarised emission at sub-arcminut…

astro-ph.GA2024

Herschel Gould Belt Survey in Taurus. II: A census of dense cores and filaments in the TMC1 region

Jason Kirk, Derek Ward-Thompson, James Di Francesco +12

We present a catalogue of dense cores and filaments in a field around the TMC1 region of the Taurus Molecular Cloud. The catalogue was created using…

astro-ph.GA2024★ 42 cited

Testing kinematic distances under a realistic Galactic potential

Glen H. Hunter, Mattia C. Sormani, Jan P. Beckmann +15

Obtaining reliable distance estimates to gas clouds within the Milky Way is challenging in the absence of certain tracers. The kinematic distance approach has been used as an alter…

astro-ph.GA2024★ 10 cited

Cloud properties across spatial scales in simulations of the interstellar medium

Tine Colman, Noé Brucy, Philipp Girichidis +9

Molecular clouds (MC) are structures of dense gas in the interstellar medium (ISM), that extend from ten to a few hundred parsecs and form the main gas reservoir available for star…