Perturbations by Mass Loss in the Orbital Elements of γ Persei and α Centauri

Details Perturbations by Mass Loss in the Orbital Elements of γ Persei and α Centauri Perturbations by Mass Loss in the Orbital Elements of γ Persei and α Centauri

Oct 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001rmxaa..37..179l&link_type=abstract

Revista Mexicana de Astronomia y Astrofisica, Vol. 37, pp. 179-186 (2001)

Astronomy and Astrophysics

Astronomy

Scientific paper

Prieto and Docobo's approach to the two-body problem with isotropic mass
loss is used to study the dynamical evolution of the orbital elements of
the binaries γ Persei and α Centauri under the assumption
that mass losses obey the Eddington-Jeans law, with separate parameters
for each component of the binaries.

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