The Restricted Three -Body Problem. Comments on the `Spatial' Equilibrium Points

Details The Restricted Three -Body Problem. Comments on the `Spatial' Equilibrium Points The Restricted Three -Body Problem. Comments on the `Spatial' Equilibrium Points

Mar 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001ap%26ss.275..425r&link_type=abstract

Astrophysics and Space Science, v. 275, Issue 4, p. 425-429 (2001).

Astronomy and Astrophysics

Astrophysics

3

Scientific paper

In the photogravitational restricted three-body problem, the role of the radiation-pressure is reviewed. By the analytical considerations, the existence of the `spatial' equilibrium points is analysed. In order to avoid the unknown parameters of the infinitesimal body, for the two component stars an analytical function β_2 =f(β_1 ) is established. In contrast to results given by other authors, here only one pair of such points is found. A numerical simulation for RW Monocerotis is undertaken and it is found L_6(-0.055 0; +1.07) and L_7(-0.055 0; -1.07).

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