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- W3150950760 abstract "differed by more than 20 km/sec. The results gave 20 percent for all main-sequence stars and somewhat less for giants and supergiants. Petrie (1960) discussed the percentage of the spectroscopic binaries from another point of view and reached different conclusions. He considered three groups, of about 500 stars each, of B, A, and F5-M objects for which at least three individual radial velocities existed. He established then the observed dispersion of the individual velocities and subtracted from this the distribution of" @default.
- W3150950760 created "2021-04-13" @default.
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- W3150950760 date "2016-01-01" @default.
- W3150950760 modified "2023-09-27" @default.
- W3150950760 title "THE FREQUENCY OF SPECTROSCOPIC BINARIES" @default.
- W3150950760 hasPublicationYear "2016" @default.
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