PHOTOMETRIC CLASSIFICATION OF THE MARGONI & STAGNI SUSPECTED VARIABLES V 58, V91
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 sta...
Main Authors: | , , |
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Format: | Article |
Language: | English |
Published: |
Odessa I. I. Mechnykov National University
2017-06-01
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Series: | Odessa Astronomical Publications |
Online Access: | http://oap.onu.edu.ua/article/view/105710 |