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SPH simulations of clumps formation by dissipative collisions of molecular clouds - II. Magnetic case
(Edp Sciences S A, 2001-12-01)
We performed computer simulations of interstellar cloud-cloud collisions using the three-dimensional smoothed particle magnetohydrodynamics method. In order to study the role of the magnetic field on the process of ...
SPH simulations of clumps formation by dissipative collisions of molecular clouds - II. Magnetic case
(Edp Sciences S A, 2001-12-01)
We performed computer simulations of interstellar cloud-cloud collisions using the three-dimensional smoothed particle magnetohydrodynamics method. In order to study the role of the magnetic field on the process of ...
Statistical tracing of magnetic fields: comparing and improving the techniques
(IOP Publishing, 2020)
The density-magnetic field relation in the atomic ISM
(Wiley Blackwell Publishing, Inc, 2018-07)
We present numerical experiments aimed to study the correlation between the magnetic field strength, B, and the density, n, in the cold atomic interstellar medium (CNM). We analyse 24 magnetohydrodynamic models with different ...
Magnetic field components analysis of the SCUPOL 850μm polarization data catalog
(Chicago, 2013)
We present an extensive analysis of the 850 μm polarization maps of the SCUBA Polarimeter Legacy (SCUPOL) Catalogue produced by Matthews et al., focusing exclusively on the molecular clouds and star-forming regions. For ...
THE ROLE OF TURBULENT MAGNETIC RECONNECTION IN THE FORMATION OF ROTATIONALLY SUPPORTED PROTOSTELLAR DISKS
(IOP PUBLISHING LTDBRISTOL, 2012)
The formation of protostellar disks out of molecular cloud cores is still not fully understood. Under ideal MHD conditions, the removal of angular momentum from the disk progenitor by the typically embedded magnetic field ...
The influence of magnetic field on the cold neutral medium mass fraction and its alignment with density structures
(Wiley Blackwell Publishing, Inc, 2018-06)
To contribute to the understanding of the magnetic field's influence on the segregation of cold neutral medium (CNM) in the solar neighbourhood we analyse magnetohydrodynamic simulations that include themain physical ...
VELOCITY FIELD OF COMPRESSIBLE MAGNETOHYDRODYNAMIC TURBULENCE: WAVELET DECOMPOSITION AND MODE SCALINGS
(IOP PUBLISHING LTD, 2010)
We study compressible magnetohydrodynamic turbulence, which holds the key to many astrophysical processes, including star formation and cosmic-ray propagation. To account for the variations of the magnetic field in the ...