Odessa Astronomical Publications (Jun 2017)

PHOTOMETRIC CLASSIFICATION OF THE MARGONI & STAGNI SUSPECTED VARIABLES V 58, V91

  • I. L. Andronov,
  • A. V. Chikrigin,
  • G. N. Kimeridze

DOI
https://doi.org/10.18524/1810-4215.1994.7.105710
Journal volume & issue
Vol. 7, no. 1
pp. 89 – 90

Abstract

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V58 was found to be an eclipsing variable with P = 0.46771d(82), TMin = 2446421.795(5) and eclipse duration d ≈ 0.2P. V91 is a RRab type star with P = 0.3493d(11), T0 = 2446421.402(5), Max=13.32m, Min=14.21m, and an asymmetry f = 0.26(2). Finding charts with photographic magnitudes of comparison stars are presented.