Spectroscopic binary orbits from photoelectric radial velocities. Paper 62: EZ Pegasi

Details Spectroscopic binary orbits from photoelectric radial velocities. Paper 62: EZ Pegasi Spectroscopic binary orbits from photoelectric radial velocities. Paper 62: EZ Pegasi

Jun 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985obs...105...81g&link_type=abstract

The Observatory, vol. 105, p. %81G-85 (1985)

Astronomy and Astrophysics

Astronomy

5

Scientific paper

EZ Peg, which has had a confused history in the astronomical literature,
is shown to be a double-lined spectroscopic binary with slightly unequal
components (both late-G dwarfs) in a circular orbit of period 11.66
days.

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