21 citations · 113 across the 20 of their papers we have counts for
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Properties of interstellar wind leading to shape morphology of the dust surrounding HD 61005
P. Pastor
A structure formed by dust particles ejected from the debris ring around HD 61005 is observed in the scattered light. The main aim here is to constrain interstellar wind parameters…
Linearized averaged resonant equations and their solution for dust particles
Pavol Pastor
The averaged resonant equations of motion for the planar circular restricted three-body problem are solved on the linearization basis taking into account also non-gravitational eff…
Locations of stationary/periodic solutions in mean motion resonances according to properties of dust grains
Pavol Pastor
The equations of secular evolution for dust grains in mean motion resonances with a planet are solved for stationary points. This is done including both Poynting-Robertson effect a…
Positions of equilibrium points for dust particles in the circular restricted three-body problem with radiation
P. Pastor
For a body with negligible mass moving in the gravitational field of a star and one planet in a circular orbit (the circular restricted three-body problem) five equilibrium points…
On the stability of dust orbits in mean motion resonances with considered perturbation from an interstellar wind
P. Pastor
Circumstellar dust particles can be captured in a mean motion resonance with a planet and simultaneously be affected by non-gravitational effects. It is possible to describe the se…
Dust particles in mean motion resonances influenced by an interstellar gas flow
P. Pastor
The orbital evolution of a dust particle captured in a mean motion resonance with a planet in circular orbit under the action of the Poynting-Robertson effect, radial stellar wind…