SPECTROSCOPIC STUDY OF LONG PERIOD ECLIPSIING BINARY 32 CYGNI

  • 발행 : 1992.12.01

초록

Spectra of the $\zeta$ Aurigae type eclipsing binary system 32 Cygni were taken at the Asiago Observatory. Using the Gaussian fitting method we can estimate the radial velocity and equivalent widths of some metalic lines.

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