The impact of turbulence and magnetic field orientation on star-forming filaments
D Seifried, S Walch - Monthly Notices of the Royal Astronomical …, 2015 - academic.oup.com
We present simulations of collapsing filaments studying the impact of turbulence and
magnetic field morphologies on their evolution and star formation properties. We vary the …
magnetic field morphologies on their evolution and star formation properties. We vary the …
Morphology and kinematics of filaments in the Serpens and Perseus molecular clouds
Abstract We present H 13 CO+(J= 1–0) and HNC (J= 1–0) maps of regions in Serpens
South, Serpens Main, and NGC 1333 containing filaments. We also observe the Serpens …
South, Serpens Main, and NGC 1333 containing filaments. We also observe the Serpens …
Studying magnetic fields and dust in M17 using polarized thermal dust emission observed by SOFIA/HAWC+
We report on the highest spatial resolution measurement to date of magnetic fields (B-fields)
in M17 using thermal dust polarization measurements taken by SOFIA/HAWC+ centered at a …
in M17 using thermal dust polarization measurements taken by SOFIA/HAWC+ centered at a …
Observations of magnetic fields surrounding LkHα 101 taken by the BISTRO survey with JCMT-POL-2
We report the first high spatial resolution measurement of magnetic fields surrounding LkHα
101, part of the Auriga–California molecular cloud. The observations were taken with the …
101, part of the Auriga–California molecular cloud. The observations were taken with the …
Alignment and rotational disruption of dust grains in the Galactic Centre revealed by polarized dust emission
MS Akshaya, T Hoang - Monthly Notices of the Royal …, 2023 - academic.oup.com
We study the alignment and rotational disruption of dust grains at the centre of our Galaxy
using polarized thermal dust emission observed by SOFIA/HAWC+ and JCMT/SCUPOL at …
using polarized thermal dust emission observed by SOFIA/HAWC+ and JCMT/SCUPOL at …
A Wide-field CO Survey toward the California Molecular Filament
W Guo, X Chen, J Feng, L Sun, C Wang… - The Astrophysical …, 2021 - iopscience.iop.org
We present the survey of 12 CO/13 CO/C 18 O (J= 1− 0) toward the California molecular
cloud (CMC) within the region of 161 fdg 75≤ l≤ 167 fdg 75,− 9 fdg 5≤ b≤− 7 fdg 5 using …
cloud (CMC) within the region of 161 fdg 75≤ l≤ 167 fdg 75,− 9 fdg 5≤ b≤− 7 fdg 5 using …
The relationship between the dust and gas-phase co across the California molecular cloud
We present results of an extinction-CO line survey of the southeastern part of the California
molecular cloud (CMC). Deep, wide-field, near-infrared images were used to construct a …
molecular cloud (CMC). Deep, wide-field, near-infrared images were used to construct a …
Filament rotation in the California L1482 cloud
Filament Rotation in the California L1482 Cloud - IOPscience This site uses cookies. By
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Physical properties and chemical composition of the cores in the California molecular cloud
GY Zhang, JL Xu, AI Vasyunin, DA Semenov… - Astronomy & …, 2018 - aanda.org
Aims. We aim to reveal the physical properties and chemical composition of the cores in the
California molecular cloud (CMC), so as to better understand the initial conditions of star …
California molecular cloud (CMC), so as to better understand the initial conditions of star …
Magnetohydrodynamical simulation of the formation of clumps and filaments in quiescent diffuse medium by thermal instability
CJ Wareing, JM Pittard, S Falle… - Monthly Notices of the …, 2016 - academic.oup.com
We have used the adaptive mesh refinement hydrodynamic code, mg, to perform idealized
3D magnetohydrodynamical simulations of the formation of clumpy and filamentary structure …
3D magnetohydrodynamical simulations of the formation of clumpy and filamentary structure …