Equilibrium and collapse of rotating, axisymmetric, idealized interstellar gas clouds is calculated with a 2D hydrodynamics code. The hydrodynamics features an improved angular momentum advection algorithm. Angular momentum is advected consistently with mass by deriving angular momentum fluxes from mass fluxes and the local distribution of specific angular momentum. Local conservation is checked by a graph of mass versus specific angular momentum for the cloud as a whole
The means by which parent molecular clouds give birth to stars constitutes a fundamental unsolved pr...
We study the self-similar collapse of an isothermal magnetized rotating cloud in the ideal magnetohy...
International audienceContext: Recent progress and constraints brought by helio and asteroseismology...
Interstellar clouds play a key role in many astrophysical events. The interactions of dense interste...
This thesis presents numerical investigations of interstellar gas under various conditions. Discrete...
In this paper we systematically investigate the length and time scales of an interstellar molecular ...
94 p.Thesis (Ph.D.)--University of Illinois at Urbana-Champaign, 1983.The formulation of a theory of...
We review the equilibrium structure of rotating isothermal clouds. First, we describe the equilibriu...
In this paper we systematically investigate the length and time scales of an interstellar molecular ...
Using hydrodynamic simulations we investigate the rotational properties and angular momentum evolut...
Context. Theoretical studies of collapsing clouds have found that even a relatively weak magnetic fi...
Numerical simulations of the collapse of a slowly rotating cloud have been performed, assuming eithe...
In this work the understanding of the rotational equilibrium of C2 in interstellar clouds is updated...
Computer experiments of interstellar cloud collisions were performed with a new smoothed-particle-hy...
Aims. We investigate the influence of turbulent viscosity on the collapse of a rotating mo...
The means by which parent molecular clouds give birth to stars constitutes a fundamental unsolved pr...
We study the self-similar collapse of an isothermal magnetized rotating cloud in the ideal magnetohy...
International audienceContext: Recent progress and constraints brought by helio and asteroseismology...
Interstellar clouds play a key role in many astrophysical events. The interactions of dense interste...
This thesis presents numerical investigations of interstellar gas under various conditions. Discrete...
In this paper we systematically investigate the length and time scales of an interstellar molecular ...
94 p.Thesis (Ph.D.)--University of Illinois at Urbana-Champaign, 1983.The formulation of a theory of...
We review the equilibrium structure of rotating isothermal clouds. First, we describe the equilibriu...
In this paper we systematically investigate the length and time scales of an interstellar molecular ...
Using hydrodynamic simulations we investigate the rotational properties and angular momentum evolut...
Context. Theoretical studies of collapsing clouds have found that even a relatively weak magnetic fi...
Numerical simulations of the collapse of a slowly rotating cloud have been performed, assuming eithe...
In this work the understanding of the rotational equilibrium of C2 in interstellar clouds is updated...
Computer experiments of interstellar cloud collisions were performed with a new smoothed-particle-hy...
Aims. We investigate the influence of turbulent viscosity on the collapse of a rotating mo...
The means by which parent molecular clouds give birth to stars constitutes a fundamental unsolved pr...
We study the self-similar collapse of an isothermal magnetized rotating cloud in the ideal magnetohy...
International audienceContext: Recent progress and constraints brought by helio and asteroseismology...
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