Magnetic fields in star formation: from clouds to cores
In this chapter we review recent advances in understanding the roles that magnetic fields
play throughout the star formation process, gained through observations and simulations of …
play throughout the star formation process, gained through observations and simulations of …
Nature of striation in 21 cm channel Maps: velocity caustics
The alignment of striated intensity structures in thin neutral hydrogen (H i) spectroscopic
channels with Galactic magnetic fields has been observed. However, the origin and nature …
channels with Galactic magnetic fields has been observed. However, the origin and nature …
Three-dimensional magnetic fields of molecular clouds
M Tahani - Frontiers in Astronomy and Space Sciences, 2022 - frontiersin.org
To investigate the role of magnetic fields in the evolution of the interstellar medium,
formation and evolution of molecular clouds, and ultimately the formation of stars, their three …
formation and evolution of molecular clouds, and ultimately the formation of stars, their three …
A Census of Outflow to Magnetic Field Orientations in Nearby Molecular Clouds
D Xu, SSR Offner, R Gutermuth… - The Astrophysical …, 2022 - iopscience.iop.org
We define a sample of 200 protostellar outflows showing blue-and redshifted CO emission
in the nearby molecular clouds Ophiuchus, Taurus, Perseus, and Orion, to investigate the …
in the nearby molecular clouds Ophiuchus, Taurus, Perseus, and Orion, to investigate the …
The JCMT BISTRO-2 Survey: Magnetic fields of the massive DR21 filament
We present 850 μm dust polarization observations of the massive DR21 filament from the B-
fields In STar-forming Region Observations (BISTRO) survey, using the POL-2 polarimeter …
fields In STar-forming Region Observations (BISTRO) survey, using the POL-2 polarimeter …
B-fields in Star-forming Region Observations (BISTRO): Magnetic fields in the filamentary structures of Serpens Main
We present 850 μm polarimetric observations toward the Serpens Main molecular cloud
obtained using the POL-2 polarimeter on the James Clerk Maxwell Telescope as part of the …
obtained using the POL-2 polarimeter on the James Clerk Maxwell Telescope as part of the …
B-fields and Dust in Interstellar Filaments Using Dust Polarization (BALLAD-POL). I. The Massive Filament G11. 11–0.12 Observed by SOFIA/HAWC+
We report the first measurement of polarized thermal dust emission toward the entire
infrared dark cloud G11. 11− 0.12 taken by the polarimeter SOFIA/HAWC+ at 214 μm. The …
infrared dark cloud G11. 11− 0.12 taken by the polarimeter SOFIA/HAWC+ at 214 μm. The …
CARMA-NRO Orion Survey: unbiased survey of dense cores and core mass functions in Orion A
H Takemura, F Nakamura, HG Arce… - The Astrophysical …, 2023 - iopscience.iop.org
The mass distribution of dense cores is a potential key to understanding the process of star
formation. Applying dendrogram analysis to the CARMA-NRO Orion C 18 O (J= 1–0) data …
formation. Applying dendrogram analysis to the CARMA-NRO Orion C 18 O (J= 1–0) data …
Mapping the Galactic magnetic field orientation and strength in three dimensions
Y Hu, A Lazarian - Monthly Notices of the Royal Astronomical …, 2023 - academic.oup.com
The mapping of the Galactic magnetic field (GMF) in three dimensions is essential to
comprehend various astrophysical processes that occur within the Milky Way. This study …
comprehend various astrophysical processes that occur within the Milky Way. This study …
Characterizing three-dimensional magnetic field, turbulence, and self-gravity in the star-forming region L1688
Y Hu, A Lazarian - Monthly Notices of the Royal Astronomical …, 2023 - academic.oup.com
Interaction of three-dimensional magnetic fields, turbulence, and self-gravity in the molecular
cloud is crucial in understanding star formation but has not been addressed so far. In this …
cloud is crucial in understanding star formation but has not been addressed so far. In this …