ADS3230 - Two Possible Solutions in the Computation of the Orbital Elements

Details ADS3230 - Two Possible Solutions in the Computation of the Orbital Elements ADS3230 - Two Possible Solutions in the Computation of the Orbital Elements

Oct 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982a%26as...50...19s&link_type=abstract

Astronomy and Astrophysics Supplement, Vol.50, P. 19, 1982

Astronomy and Astrophysics

Astrophysics

Scientific paper

Orbital elements of the visual binary star ADS 3230 are given. Two solutions are possible if the observations preceding the 1925 are considered in the second or in the fourth quadrant.
The first group of elements, with period of 217 years, leads to a total mass of the system of 2.23 Msun the other, with period of 856.7 years, more uncertain than the previous one, gives a total mass of the system of 5.03 Msun and is more reliable from an astrophysical point of view.

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