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Modelling [C I] emission from turbulent molecular clouds
(Royal Astronomical Society, 2015)
We use detailed numerical simulations of a turbulent molecular cloud to study the usefulness
of the [CI] 609 and 370 μmfine structure emission lines as tracers of cloud structure. Emission
from these lines is observed ...
Modelling [CI] emission from turbulent molecular clouds
(Oxford University Press, 2015)
© 2015 The Authors.We use detailed numerical simulations of a turbulent molecular cloud to study the usefulness of the [CI] 609 and 370 μmfine structure emission lines as tracers of cloud structure. Emission from these ...
THE COLLAPSE OF TURBULENT CORES AND RECONNECTION DIFFUSION
(Iop Publishing LtdBristolInglaterra, 2013)
DIFFUSION OF MAGNETIC FIELD AND REMOVAL OF MAGNETIC FLUX FROM CLOUDS VIA TURBULENT RECONNECTION
(IOP PUBLISHING LTD, 2010)
The diffusion of astrophysical magnetic fields in conducting fluids in the presence of turbulence depends on whether magnetic fields can change their topology via reconnection in highly conducting media. Recent progress ...
The role of reconnection diffusion in the gravitational collapse of turbulent cloud cores
(International Astronomical UnionFlorianópolis, 2013)
For a molecular cloud clump to form stars some
transport of magnetic flux is required from the
denser, inner regions to the outer regions of the
cloud, otherwise this can prevent the collapse. Fast
magnetic reconnection ...
Estudio de la evolución de diferentes nubes protoestelares en simulaciones
(2021-03)
El proceso de formación estelar es aún uno de los principales problemas sin resolver de la astrofísica moderna. A pesar de que el conocimiento acerca de este proceso fundamental, conectado a las áreas de formación galáctica, ...
Rotation in molecular clouds
(1999)
We have investigated a broad range of evidence concerning rotation in molecular clouds. As a consequence, we show that trends in specific angular momentum J/M and angular velocity ? are inconsistent with certain models of ...