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Cen X-3 as Seen by Maxi During Six Years

The aim of this work is to study both light curve and orbital phase spectroscopy of Cen X-3 taking advantage of the MAXI/GSC observation strategy. These studies allow delimiting the stellar wind properties and its interactions with the compact object. From the analysis of the light curve, we have es...

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Publicat a:Revista Mexicana de Astronomía y Astrofísica
Autors principals: Á. Torregrosa, J. J. Rodes-Roca, J. M. Torrejón, G. Sanjurjo-Ferrín, G. Bernabéu
Format: Artigo
Idioma:Inglês
Publicat: Universidad Nacional Autónoma de México 2022
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Accés en línia:https://www.redalyc.org/articulo.oa?id=57175502015
https://www.redalyc.org/journal/571/57175502015/
https://www.redalyc.org/journal/571/57175502015/html/
https://www.redalyc.org/journal/571/57175502015/57175502015.epub
https://www.redalyc.org/journal/571/57175502015/movil
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