Dynamics of dust around a rotating star

Details Dynamics of dust around a rotating star Dynamics of dust around a rotating star

May 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26a...245..199b&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 245, no. 1, May 1991, p. 199-202. CICYT-supported research.

Astronomy and Astrophysics

Astrophysics

2

Electromagnetic Radiation, Gravitational Effects, Stellar Envelopes, Stellar Rotation, Circular Orbits, Equations Of Motion, Interplanetary Medium, Kepler Laws, Stellar Luminosity

Scientific paper

The orbital evolution of dust particles initially located outside the
equatorial plane is considered. The averaging method is used to solve
equations of motion. It is concluded that dust particles move in
circular orbits perpendicular to the rotational axis and that the radius
of these orbits depends on particle size and star luminosity.

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