A STUDY OF THE SECULAR VARIATION OF THE HIGH-AMPLITUDE DELTA SCUTI STAR AD CMI
| dc.contributor.author | J. H. Peña | |
| dc.contributor.author | Douglas dos Santos Pina | |
| dc.contributor.author | H. Huepa | |
| dc.contributor.author | Sergio B. Juárez | |
| dc.contributor.author | C. Villarreal | |
| dc.contributor.author | J. Guillén | |
| dc.contributor.author | A. A. Soní | |
| dc.contributor.author | A. Rentería | |
| dc.contributor.author | J. M. Donaire | |
| dc.contributor.author | Ricardo R. Muñoz | |
| dc.coverage.spatial | Bolivia | |
| dc.date.accessioned | 2026-03-22T18:35:10Z | |
| dc.date.available | 2026-03-22T18:35:10Z | |
| dc.date.issued | 2021 | |
| dc.description.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. | |
| dc.identifier.doi | 10.22201/ia.01851101p.2021.57.02.06 | |
| dc.identifier.uri | https://doi.org/10.22201/ia.01851101p.2021.57.02.06 | |
| dc.identifier.uri | https://andeanlibrary.org/handle/123456789/70987 | |
| dc.language.iso | en | |
| dc.publisher | National Autonomous University of Mexico | |
| dc.relation.ispartof | Revista Mexicana de Astronomía y Astrofísica | |
| dc.source | Universidad Nacional Autónoma de México | |
| dc.subject | Physics | |
| dc.subject | Photometry (optics) | |
| dc.subject | Delta | |
| dc.subject | Amplitude | |
| dc.subject | Astrophysics | |
| dc.subject | Variation (astronomy) | |
| dc.subject | Photoelectric effect | |
| dc.subject | Star (game theory) | |
| dc.subject | Astronomy | |
| dc.subject | Stars | |
| dc.title | A STUDY OF THE SECULAR VARIATION OF THE HIGH-AMPLITUDE DELTA SCUTI STAR AD CMI | |
| dc.type | article |