A study of the secular variation of the high-amplitude Delta Scuti star AD CMi

Peña, J. H.; Piña, D. S.; Huepa, H.; Juárez, S. B.; Villarreal, C.; Guillén, J.; Soni, A. A.; Rentería, A.; Donaire, J. M.; Muñoz, R. R.; Benadalid, T.; Paredes, J. D.; Orozco, E. D.; Soberanes, I.; Posadas, H.; Castro, C.; Briones, J.; Romero, M.; Martinez, F.; Zuñiga, A. L.; Carrillo, J. L.; Chávez, B.; Navez, D.; García, C.

doi:10.22201/ia.01851101p.2021.57.02.06

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Revista mexicana de astronomía y astrofísica

Print version ISSN 0185-1101

Abstract

PENA, J. H. et al. A study of the secular variation of the high-amplitude Delta Scuti star AD CMi. Rev. mex. astron. astrofis [online]. 2021, vol.57, n.2, pp.321-334. Epub Feb 15, 2022. ISSN 0185-1101. https://doi.org/10.22201/ia.01851101p.2021.57.02.06.

We determine the nature of the Delta Scuti star AD CMi and its physical parameters from newly determined times of maximum light and other times from the literature, as well as from uvby − β photoelectric photometry.

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