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20092026
most citedFirst results from BISTRO -- a SCUBA-2 polarimeter survey of the Gould Belt

134 citations · 1.4k across the 58 of their papers we have counts for

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astro-ph.SR2024

Magnetic Fields in Massive Star-forming Regions (MagMaR) IV: Tracing the Magnetic Fields in the O-type protostellar system IRAS 165474247

Luis A. Zapata, Manuel Fernández-López, Patricio Sanhueza +24

The formation of the massive stars, and in particular, the role that the magnetic fields play in their early evolutionary phase is still far from being completely understood. Here,…

astro-ph.SR2024

Filamentary Network and Magnetic Field Structures Revealed with BISTRO in the High-Mass Star-Forming Region NGC2264 : Global Properties and Local Magnetogravitational Configurations

Jia-Wei Wang, Patrick M. Koch, Seamus D. Clarke +154

We report 850 m continuum polarization observations toward the filamentary high-mass star-forming region NGC 2264, taken as part of the B-fields In STar forming Regions Observat…

astro-ph.SR2022

Effects of magnetic field orientations in dense cores on gas kinematics in protostellar envelopes

Aashish Gupta, Hsi-Wei Yen, Patrick Koch +16

Theoretically, misalignment between the magnetic field and rotational axis in a dense core is considered to be dynamically important in the star formation process, however, extent…

astro-ph.SR2017★ 68 cited

How do stars gain their mass? A JCMT/SCUBA-2 Transient Survey of Protostars in Nearby Star Forming Regions

Gregory J. Herczeg, Doug Johnstone, Steve Mairs +55

Most protostars have luminosities that are fainter than expected from steady accretion over the protostellar lifetime. The solution to this problem may lie in episodic mass accreti…