New Double Periodic Variable Stars in the ASAS-SN Catalog
J. A. Rosales, R. E. Mennickent

TL;DR
This paper reports the discovery of three new double periodic variable stars identified through analysis of ASAS-SN light curves, expanding the catalog of such variables with specific orbital and long cycle periods.
Contribution
The study introduces three newly identified double periodic variables with detailed period measurements, utilizing light curve analysis from the ASAS-SN survey.
Findings
Discovered 3 new double periodic variables.
Orbital periods range from 10 to 20 days.
Long cycles range from 300 to 600 days.
Abstract
We report the discovery of 3 new Double Periodic Variables based on the analysis of ASAS-SN light curves: GSD J11630570-510306, V593 Sco and TYC 6939-678-1. These systems have orbital periods between 10 and 20 days and long cycles between 300 and 600 days.
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