Triple Star Parameters and Masses

Details Triple Star Parameters and Masses Triple Star Parameters and Masses

Aug 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997esasp.402..425s&link_type=abstract

Proceedings of the ESA Symposium `Hipparcos - Venice '97', 13-16 May, Venice, Italy, ESA SP-402 (July 1997), p. 425-428

Computer Science

1

Scientific paper

A non-negligible number of orbital visual binaries, suitable for mass-determination using the Hipparcos parallaxes, are members of visual multiple systems. The extra component(s) were not always taken into account in the standard Hipparcos reductions, but starting from the intermediate `Transit Data', supplemented by speckle interferometry and/or reliable earlier orbits, it it possible to make more complete use of the Hipparcos data. A few examples of such combined triple star solutions are given, including new mass-determinations for the close pair.

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