Die sekundare Periode von RV Arietis

Details Die sekundare Periode von RV Arietis Die sekundare Periode von RV Arietis

Jan 1956

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1956cokon..40....1d&link_type=abstract

Communications of the Konkoly Observatory, No. 40-41 (Vol. III, 21), p. 1-7 (1956).

Physics

2

Stars: Luminosity Function

Scientific paper

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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