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20002022
most citedClouds, filaments and protostars: the Herschel Hi-GAL Milky Way

806 citations · 8k across the 121 of their papers we have counts for

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Showing 2014 · astro-ph.GAShow all

9 papers · 2 filters

astro-ph.GA2014★ 60 cited

The Importance of the Magnetic Field from an SMA-CSO-Combined Sample of Star-Forming Regions

Patrick M. Koch, Ya-Wen Tang, Paul T. P. Ho +14

Submillimeter dust polarization measurements of a sample of 50 star-forming regions, observed with the SMA and the CSO covering pc-scale clouds to mpc-scale cores, are analyzed in…

astro-ph.GA2014★ 80 cited

Submillimeter Array Observations of Magnetic Fields in G240.31+0.07: an Hourglass in a Massive Cluster-forming Core

Keping Qiu, Qizhou Zhang, Karl M. Menten +3

We report the first detection of an hourglass magnetic field aligned with a well-defined outflow-rotation system in a high-mass star-forming region. The observations were performed…

astro-ph.GA2014★ 209 cited

Magnetic Fields and Massive Star Formation

Qizhou Zhang, Keping Qiu, Josep M. Girart +17

Massive stars ( \msun) typically form in parsec-scale molecular clumps that collapse and fragment, leading to the birth of a cluster of stellar objects. We investigate the r…

astro-ph.GA2014★ 86 cited

VLA observations of ammonia in high-mass star formation regions

Xing Lu, Qizhou Zhang, Hauyu Baobab Liu +2

We report systematic mapping observations of the NH (1,1) and (2,2) inversion lines towards 62 high-mass star-forming regions using VLA in its D and DnC array configurations.…

astro-ph.GA2014★ 98 cited

ALMA Results of the Pseudodisk, Rotating disk, and Jet in Continuum and HCO+ in the Protostellar System HH 212

Chin-Fei Lee, Naomi Hirano, Qizhou Zhang +3

HH 212 is a nearby (400 pc) Class 0 protostellar system showing several components that can be compared with theoretical models of core collapse. We have mapped it in 350 GHz conti…

astro-ph.GA2014★ 22 cited

A sub-arcsecond study of the hot molecular core in G023.01-00.41

A. Sanna, R. Cesaroni, L. Moscadelli +5

(Abridged) METHODS: We performed SMA observations at 1.3 mm with both the most extended and compact array configurations, providing sub-arcsecond and high sensitivity maps of vario…

astro-ph.GA2014★ 264 cited

Hierarchical fragmentation and differential star formation in the Galactic "Snake": infrared dark cloud G11.11-0.12

Ke Wang, Qizhou Zhang, Leonardo Testi +8

We present Submillimeter Array (SMA) 0.88 and 1.3 mm broad band observations, and the Jansky Very Large Array (VLA) observations in up to ,…

astro-ph.GA2014★ 101 cited

Fragmentation of massive dense cores down to ~1000 AU: Relation between fragmentation and density structure

Aina Palau, R. Estalella, J. M. Girart +10

In order to shed light on the main physical processes controlling fragmentation of massive dense cores, we present a uniform study of the density structure of 19 massive dense core…

astro-ph.GA2014★ 46 cited

Star Cluster Formation and Feedback

Mark R. Krumholz, Matthew R. Bate, Hector G. Arce +6

Stars do not generally form in isolation. Instead, they form in clusters, and in these clustered environments newborn stars can have profound effects on one another and on their pa…