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Autor:
Rodríguez-Segovia, N., Hajdu, G., Catelan, M., Espinoza-Arancibia, F., Boggiano, G., Cenzano, C., H., E. Garcés, Joachimi, K., Muñoz-López, C., Ordenes-Huanca, C., Orquera-Rojas, C., Torres, P., Valenzuela-Navarro, Á.
The period-change rate (PCR) of pulsating variable stars is a useful probe of changes in their interior structure, and thus of their evolutionary stages. So far, the PCRs of Classical Cepheids in the Large Magellanic Cloud (LMC) have been explored in
Externí odkaz:
http://arxiv.org/abs/2111.03503
