245 citations · 3.3k across the 48 of their papers we have counts for
48 papers
SOFIA and ALMA Investigate Magnetic Fields and Gas Structures in Massive Star Formation: The Case of the Masquerading Monster in BYF 73
Peter J. Barnes, Stuart D. Ryder, Giles Novak +4
We present SOFIA+ALMA continuum and spectral-line polarisation data on the massive molecular cloud BYF 73, revealing important details about the magnetic field morphology, gas stru…
ALMA CN Zeeman Observations of AS 209: Limits on Magnetic Field Strength and Magnetically Driven Accretion Rate
Rachel E. Harrison, Leslie W. Looney, Ian W. Stephens +7
While magnetic fields likely play an important role in driving the evolution of protoplanetary disks through angular momentum transport, observational evidence of magnetic fields h…
Review of Zeeman Effect Observations of Regions of Star Formation
Richard M. Crutcher, Athol J. Kemball
(Edited for length) The Zeeman effect is the only observational technique available to measure directly the strength of magnetic fields in regions of star formation. We review the…
The seven most massive clumps in W43-Main as seen by ALMA: Dynamical equilibrium and Magnetic Fields
Paulo C. Cortes, Charles L. H. Hull, Josep M. Girart +8
Here we present new ALMA observations of polarized dust emission from six of the most massive clumps in W43-Main. The clumps MM2, MM3, MM4, MM6, MM7, and MM8, have been resolved in…
HAWC+/SOFIA Multiwavelength Polarimetric Observations of OMC-1
David T. Chuss, B-G Andersson, John Bally +35
We report new polarimetric and photometric maps of the massive star-forming region OMC-1 using the HAWC+ instrument on the Stratospheric Observatory for Infrared Astronomy (SOFIA).…
ALMA Reveals Transition of Polarization Pattern with Wavelength in HL Tau's Disk
Ian W. Stephens, Haifeng Yang, Zhi-Yun Li +10
The mechanism for producing polarized emission from protostellar disks at (sub)millimeter wavelengths is currently uncertain. Classically, polarization is expected from non-spheric…