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

ABSTRACT 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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Bibliographic Details
Main Authors: 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.
Format: Digital revista
Language:English
Published: Universidad Nacional Autónoma de México, Instituto de Astronomía 2021
Online Access:http://www.scielo.org.mx/scielo.php?script=sci_arttext&pid=S0185-11012021000200321
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