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Analysis of a short periodic pulsator: SX phoenicis star XX Cyg

Photometric observations were made of the SX Phoenicis star XX Cyg between September and October 2019, using the 1.88-m Kottamia reflector telescope in Egypt. We used 340 CCD observations with blue-visible-red (BVR) filters to derive light curves. In addition, we obtained 9540 visual magnitudes for...

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Bibliografische Detailangaben
Veröffentlicht in:Revista Mexicana de Astronomía y Astrofísica
Hauptverfasser: Mohamed Abdel-Sabour, Ahmed Shokry, Ahmed Ibrahim
Format: Artigo
Sprache:Inglês
Veröffentlicht: Universidad Nacional Autónoma de México 2020
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Online-Zugang:https://www.redalyc.org/articulo.oa?id=57171663010
https://www.redalyc.org/journal/571/57171663010/
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