COMMUNICATIONS / MITTEILUNGEN
L. Detre
Die sekundäre periode von RV Arietis
J. Balázs
Diskussion von 504 photographischen beobachtungen von RV Arietis
No. 40
Budapest, 1956
Abstract (Detre: Die sekundäre periode von RV Arietis)
From Broglia's and Pestarino's photoeletric and Balazs's photographic
observations the star is found to have a beat period of 0,316330d, or in units
of the primary period 3,397. This is the same value as that for AI Velorum
obtained by Walraven.
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