HAWC+/SOFIA Polarimetry in L1688: Relative Orientation of Magnetic Field and Elongated Cloud Structure

We present a study of the relative orientation between the magnetic field and elongated cloud structures for the ρ Oph A and ρ Oph E regions in L1688 in the Ophiuchus molecular cloud. Combining inferred magnetic field orientation from HAWC+ 154 μ m observations of polarized thermal emission with col...

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Veröffentlicht in:	The Astrophysical journal 2021-09, Vol.918 (1), p.39
Hauptverfasser:	Lee, Dennis, Berthoud, Marc, Chen, Che-Yu, Cox, Erin G., Davidson, Jacqueline A., Encalada, Frankie J., Fissel, Laura M., Harrison, Rachel, Kwon, Woojin, Li, Di, Li, Zhi-Yun, Looney, Leslie W., Novak, Giles, Sadavoy, Sarah, Santos, Fabio P., Segura-Cox, Dominique, Stephens, Ian
Format:	Artikel
Sprache:	eng
Schlagworte:	Alignment Astrophysics Cloud structure Clouds Computational fluid dynamics Density E region Elongated structure Fluid flow Giant molecular clouds Histograms Hydrogen Interstellar magnetic fields Interstellar medium Magnetic fields Magnetohydrodynamic simulation Magnetohydrodynamic turbulence Molecular clouds Orientation Polarimetry Star formation Thermal emission Turbulent flow
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