activity
20042020
most citedThe relation between gas and dust in the Taurus Molecular Cloud

270 citations · 3.7k across the 40 of their papers we have counts for

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Showing astro-ph.GAShow all

14 papers · 1 filter

astro-ph.GA2020★ 29 cited

The role of the magnetic field in the fragmentation process: the case of G14.225-0.506

N. Añez-López, G. Busquet, P. M. Koch +8

B-fields are predicted to play a role in the formation of filamentary structures and their fragmentation process. We aim at investigating the role of the B-field in the process of…

astro-ph.GA2019★ 79 cited

Gravity, Magnetic Field, and Turbulence: Relative Importance and Impact on Fragmentation in the Infrared Dark Cloud G34.43+00.24

Ya-Wen Tang, Patrick M. Koch, Nicolas Peretto +5

(Abbreviated) We investigate the interplay between magnetic (B) field, gravity, and turbulence in the fragmentation process of cores within the filamentary infrared dark cloud G34.…

astro-ph.GA2018★ 17 cited

Catching the Birth of a Dark Molecular Cloud for the First Time

Pei Zuo, Di Li, J. E. G. Peek +5

The majority of hydrogen in the interstellar medium (ISM) is in atomic form. The transition from atoms to molecules and, in particular, the formation of the H molecule, is a ke…

astro-ph.GA2018★ 1 cited

Magnetic Fields from Filaments to Cores

Patrick M. Koch, Ya-Wen Tang, Nicholas L. Chapman +7

How important is the magnetic (B-) field when compared to gravity and turbulence in the star-formation process? Does its importance depend on scale and location? We summarize submm…

astro-ph.GA2015★ 10 cited

First Detection of 350 Micron Polarization From a Radio-loud AGN

Sang-Sung Lee, Sincheol Kang, Do-Young Byun +5

We report the first detection of linearly polarized emission at an observing wavelength of 350 m from the radio-loud Active Galactic Nucleus 3C 279. We conducted polarization ob…

astro-ph.GA2014★ 30 cited

The Spitzer Survey of Interstellar Clouds in the Gould Belt. VI. The Auriga-California Molecular Cloud observed with IRAC and MIPS

Hannah Broekhoven-Fiene, Brenda C. Matthews, Paul M. Harvey +15

We present observations of the Auriga-California Molecular Cloud (AMC) at 3.6, 4.5, 5.8, 8.0, 24, 70 and 160 micron observed with the IRAC and MIPS detectors as part of the Spitzer…