Physics
Scientist
1 Per: a new eclipsing binary with a long period and an elliptical orbit
1 Persei, a low amplitude eclipsing binary, has a period of 25.939 days and an elliptical orbit.
133 times of maximum and first ephemeris for the RRc star VZ Draconis.
44 times of minimum and first ephemeris for the EW star FZ Orionis.
BP Pegasi: 74 times of maxima, improvement of the ephemeris and evidence of visually observed Blazhko effect.
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