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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 2011 · astro-ph.GAShow all

7 papers · 2 filters

astro-ph.GA2011★ 68 cited

Protostellar Outflow Heating in a Growing Massive Protocluster

Ke Wang, Qizhou Zhang, Yuefang Wu +2

The dense molecular clump P1 in the infrared dark cloud (IRDC) complex G28.34+0.06 harbors a massive protostellar cluster at its extreme youth. Our previous Submillimeter Array (SM…

astro-ph.GA2011★ 62 cited

Unveiling the physical properties and kinematics of molecular gas in the Antennae Galaxies (NGC 4038/9) through high resolution CO (J = 3-2) observations

Junko Ueda, Daisuke Iono, Glen Petitpas +12

We present a ~ 1" (100 pc) resolution 12CO (3-2) map of the nearby intermediate stage interacting galaxy pair NGC 4038/9 (the Antennae galaxies) obtained with the Submillimeter Arr…

astro-ph.GA2011★ 37 cited

Intermediate-mass hot cores at 500 AU: disks or outflows?

Aina Palau, Asuncion Fuente, Josep M. Girart +12

Observations with the Plateau de Bure Interferometer in the most extended configuration toward two intermediate-mass star-forming regions, IRAS22198+6336 and AFGL5142, reveal the p…

astro-ph.GA2011★ 49 cited

Structure of the hot molecular core G10.47+0.03

Rainer Rolffs, Peter Schilke, Qizhou Zhang +1

The physical structure of hot molecular cores, where forming massive stars have heated up dense dust and gas, but have not yet ionized the molecules, poses a prominent challenge in…

astro-ph.GA2011★ 158 cited

Hierarchical Fragmentation and Jet-like Outflows in IRDC G28.34+0.06, a Growing Massive Protostar Cluster

Ke Wang, Qizhou Zhang, Yuefang Wu +1

We present Submillimeter Array (SMA) λ= 0.88mm observations of an infrared dark cloud (IRDC) G28.34+0.06. Located in the quiescent southern part of the G28.34 cloud, the region of…

astro-ph.GA2011★ 60 cited

IRDC G030.88+00.13: A Tale of Two Massive Clumps

Qizhou Zhang, Ke Wang

Massive stars (M $\gsim 10$ \msun) form from collapse of parsec-scale molecular clumps. How molecular clumps fragment to give rise to massive stars in a cluster with a distribution…

astro-ph.GA2011★ 15 cited

A High Mass Dusty Disk Candidate: The Case of IRAS 18151-1208

Cassandra Fallscheer, Henrik Beuther, Jürgen Sauter +2

Many questions remain regarding the properties of disks around massive prototstars. Here we present the observations of a high mass protostellar object including an elongated dust…