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A revision of NSV 13538 = NSVS 17231162

by Alexandr Ditkovsky in March-April 2014 (#5)

Abstract: A revision of the variable star NSV 13538 is presented. Light curve elements were improved by using a modern data from photometric surveys available online. The following photometric elements of the minimum of the Long Secondary Period were found: Min = HJD 2454611 + 324 * E.
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Selected Issue (#5)

Issue #5
March-April 2014





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In this issue:
KOI-3278: A self-lensing binary star system by Ivan Adamin

BL Bootis stars - anomalous Cepheids by Ivan Adamin

A revision of NSV 13538 = NSVS 17231162 by Alexandr Ditkovsky

NSVS 11075037 = Dauban V53:
updated elements of a Mira variable in Hercules
by Siarhey Hadon

Pulsating variable stars and the Hertzsprung-Russell diagram
by Siarhey Hadon, Ivan Adamin

RS Puppis: the light echoes calibrate standard candles for accurate distance measurements
by Ivan Adamin

SS Lacertae: The non-eclipsing eclipsing binary by Ivan Adamin

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