Add to ORKGThis paper contains the calculation of the tangential component of the velocity for a model of galaxy with axial symmetry, non stationary state and equatorial symmetry plane, from the postulates and fundamental equations of Chandrasekhar theory, that shows a shift of the maximum for different values of the Z coordinate and the ¿ direction.Peer Reviewe
Context. Stars experience rapid contraction or expansion at different phases of their evolution. Mod...
In an arbitrary axisymmetric stationary spacetime, we determine the expression for the tangential ve...
© 2019 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Socie...
This paper contains the calculation of the tangential component of the velocity for a model of galax...
SIGLEAvailable from British Library Document Supply Centre- DSC:D66631/86 / BLDSC - British Library ...
Under a common potential, a finite mixture of ellipsoidal velocity distributions satisfying the Bolt...
A particular case of steady state and axial symmetry - the potentialformula proposed by Miyamoto and...
A large sample with the full space motions drawn from the Hipparcos Catalogue allows us to select so...
Abstract. We developed a numerical method for a solution of the radia-tive transfer equation in axia...
In Galactic dynamics, various assumptions have been employed for mathematical ease. These assumption...
We present a family of self-consistent axisymmetric stellar systems that have analytic distribution ...
We consider solutions with conformal symmetry of the static, spherically symmetric gravitational fie...
International audienceThis paper is the third in a series of articles devoted to the determination o...
Under a common potential, a finite mixture of ellipsoidal velocity distributions satisfyin...
Solving the Boltzmann collisionless equatio n under the axisymmetric hypot hesis introduces serious ...
Context. Stars experience rapid contraction or expansion at different phases of their evolution. Mod...
In an arbitrary axisymmetric stationary spacetime, we determine the expression for the tangential ve...
© 2019 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Socie...
This paper contains the calculation of the tangential component of the velocity for a model of galax...
SIGLEAvailable from British Library Document Supply Centre- DSC:D66631/86 / BLDSC - British Library ...
Under a common potential, a finite mixture of ellipsoidal velocity distributions satisfying the Bolt...
A particular case of steady state and axial symmetry - the potentialformula proposed by Miyamoto and...
A large sample with the full space motions drawn from the Hipparcos Catalogue allows us to select so...
Abstract. We developed a numerical method for a solution of the radia-tive transfer equation in axia...
In Galactic dynamics, various assumptions have been employed for mathematical ease. These assumption...
We present a family of self-consistent axisymmetric stellar systems that have analytic distribution ...
We consider solutions with conformal symmetry of the static, spherically symmetric gravitational fie...
International audienceThis paper is the third in a series of articles devoted to the determination o...
Under a common potential, a finite mixture of ellipsoidal velocity distributions satisfyin...
Solving the Boltzmann collisionless equatio n under the axisymmetric hypot hesis introduces serious ...
Context. Stars experience rapid contraction or expansion at different phases of their evolution. Mod...
In an arbitrary axisymmetric stationary spacetime, we determine the expression for the tangential ve...
© 2019 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Socie...