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The chemistry and kinematics of two molecular clouds near Sagittarius A*
(Oxford University Press, 2016)
We have analysed the chemical and kinematic properties of the 20 and 50 km s(-1) molecular clouds in the Central Molecular Zone of the Milky Way Galaxy, as well as those of the molecular ridge bridging these two clouds. ...
The Chemistry and Kinematics of Two Molecular Clouds near Sagittarius A
(Royal Astronomical Society, 2016-08-09)
We have analysed the chemical and kinematic properties of the 20 and 50 km s−1 molecular clouds in the Central Molecular Zone of the Milky Way Galaxy, as well as those of the molecular ridge bridging these two clouds. Our ...
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 ...
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 ...
Physical properties of molecular clouds in the southern outer Galaxy
(1997)
We have used a deep CO survey of the third galactic quadrant (May et al. 1993) to derive the physical properties of molecular clouds in the outer Galaxy. Within the range of this survey, from 194° to 270° in galactic ...