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...
Furkejuvvon:
| Publikašuvnnas: | Revista Mexicana de Astronomía y Astrofísica |
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| Váldodahkkit: | , , |
| Materiálatiipa: | Artigo |
| Giella: | Inglês |
| Almmustuhtton: |
Universidad Nacional Autónoma de México
2020
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| Fáttát: | |
| Liŋkkat: | https://www.redalyc.org/articulo.oa?id=57171663010 https://www.redalyc.org/journal/571/57171663010/ https://www.redalyc.org/journal/571/57171663010/html/ https://www.redalyc.org/journal/571/57171663010/57171663010.epub https://www.redalyc.org/journal/571/57171663010/movil |
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