Spectroscopic Binaries With Apparent Peculiar OrbitsAfter J. Miller Barr (1)
Installed on 30 Apr 2010. Latest update 1 May 2010.
This file shows a graph of computed longitudes of periastron based on a
truncated version of J. Miller Barr's (1908) table of spectroscopic binaries(1). Eight Cepheid
variables (which are currently considered to be pulsators) and three binaries for which the
eccentricity and average orbit speed were not available, have been removed from
the table.
The radial lines represent the values of ω, i.e., the computed longitude of periastron, for nineteen spectroscopic binaries. See accompanying table. |
References(2) Pourbaix, D., Resolved double-lined spectrographic binaries: A neglected source of hypothesis-free parallaxes and stellar masses, Astronomy & Astrophysics Supplement Series, 145, 215 (2000) - NADS |
Send comments/questions to Robert Fritzius at
fritzius@bellsouth.net
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