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19942026
most citedOutflow Feedback Regulated Massive Star Formation in Parsec-Scale Cluster Forming Clumps

387 citations · 7.1k across the 144 of their papers we have counts for

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Showing 2014Show all

7 papers · 1 filter

astro-ph.IM2014

Software Polarization Spectrometer "PolariS"

Izumi Mizuno, Seiji Kameno, Amane Kano +6

We have developed a software-based polarization spectrometer, PolariS, to acquire full-Stokes spectra with a very high spectral resolution of 61 Hz. The primary aim of PolariS is t…

astro-ph.IM2014★ 50 cited

The Next Generation BLAST Experiment

Nicholas Galitzki, Peter A. R. Ade, Francesco E. Angilè +38

The Balloon-borne Large Aperture Submillimeter Telescope for Polarimetry (BLASTPol) was a suborbital experiment designed to map magnetic fields in order to study their role in star…

astro-ph.IM2014★ 17 cited

The next-generation BLASTPol experiment

Bradley Dober, Peter A. R. Ade, Peter Ashton +36

The Balloon-borne Large Aperture Submillimeter Telescope for Polarimetry (BLASTPol) is a suborbital mapping experiment designed to study the role magnetic fields play in star forma…

astro-ph.SR2014★ 79 cited

Cluster Formation Triggered by Filament Collisions in Serpens South

Fumitaka Nakamura, Koji Sugitani, Tomohiro Tanaka +24

The Serpens South infrared dark cloud consists of several filamentary ridges, some of which fragment into dense clumps. On the basis of CCS (), HCN (), N$_2…

astro-ph.GA2014★ 84 cited

High abundance ratio of CO to CO toward photon-dominated regions in the Orion-A giant molecular cloud

Yoshito Shimajiri, Yoshimi Kitamura, Masao Saito +11

Aims. We derive physical properties such as the optical depths and the column densities of CO and CO to investigate the relationship between the far ultraviolet (FUV)…

astro-ph.SR2014★ 48 cited

Confronting Outflow-Regulated Cluster Formation Model with Observations

Fumitaka Nakamura, Zhi-Yun Li

Protostellar outflows have been shown theoretically to be capable of maintaining supersonic turbulence in cluster-forming clumps and keeping the star formation rate per free-fall t…