Results of Observations of Maxima of Pulsating Stars
The systematic study of some HADS stars, recognized as variables for decades, has allowed us to provide data on their secular variations through O-C analysis. However, some of the data have large gaps without observations. This is our motivation for continuously observing these stars as part of the...
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| Pubblicato in: | Revista Mexicana de Astronomía y Astrofísica |
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| Autori principali: | , , , , , , , , |
| Natura: | Artigo |
| Lingua: | Inglês |
| Pubblicazione: |
Universidad Nacional Autónoma de México
2021
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| Soggetti: | |
| Accesso online: | https://www.redalyc.org/articulo.oa?id=57171634018 https://www.redalyc.org/journal/571/57171634018/ https://www.redalyc.org/journal/571/57171634018/html/ https://www.redalyc.org/journal/571/57171634018/57171634018.epub https://www.redalyc.org/journal/571/57171634018/movil |
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