107 citations · 335 across the 12 of their papers we have counts for
12 papers
SOFIA Polarization Spectrum of Three Star-Forming Clouds
Erin G. Cox, Giles Novak, David T. Chuss +6
The dust emission polarization spectrum -- how the polarization percentage changes with wavelength -- serves as a probe of dust grain properties in star-forming regions. In this pa…
Magnetic Field Alignment Relative to Multiple Tracers in the High-mass Star-forming Region RCW 36
Akanksha Bij, Laura M. Fissel, Lars Bonne +9
We use polarization data from SOFIA HAWC+ to investigate the interplay between magnetic fields and stellar feedback in altering gas dynamics within the high-mass star-forming regio…
Modeling the Far-Infrared Polarization Spectrum of a High-Mass Star Forming Cloud
Dennis Lee, Che-Yu Chen, Giles Novak +7
The polarization spectrum, or wavelength dependence of the polarization fraction, of interstellar dust emission provides important insights into the grain alignment mechanism of in…
The Twisted Magnetic Field of the Protobinary L483
Erin G. Cox, Giles Novak, Sarah Sadavoy +16
We present H-band (1.65 m) and SOFIA HAWC+ 154 m polarization observations of the low-mass core L483. Our H-band observations reveal a magnetic field that is overwhelmingly i…
HAWC+/SOFIA Polarimetry in L1688: Relative Orientation of Magnetic Field and Elongated Cloud Structure
Dennis Lee, Marc Berthoud, Che-Yu Chen +14
We present a study of the relative orientation between the magnetic field and elongated cloud structures for the Oph A and Oph E regions in L1688 in the Ophiuchus molecular…
HAWC+ Far-Infrared Observations of the Magnetic Field Geometry in M51 and NGC 891
Terry Jay Jones, Jin-Ah Kim, C. Darren Dowell +29
SOFIA HAWC+ polarimetry at $154~\micron$ is reported for the face-on galaxy M51 and the edge-on galaxy NGC 891. For M51, the polarization vectors generally follow the spiral patter…