高振幅三角星adcmi的长期变化研究

IF 1.1 4区物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS

Revista Mexicana de Astronomia y Astrofisica Pub Date : 2021-10-01 DOI:10.22201/ia.01851101p.2021.57.02.06

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

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引用次数: 0

摘要

我们根据最新确定的最大光时间和文献中的其他时间，以及uvby - β光电光度法，确定了Delta Scuti星AD CMi的性质及其物理参数。

本文章由计算机程序翻译，如有差异，请以英文原文为准。

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A STUDY OF THE SECULAR VARIATION OF THE HIGH-AMPLITUDE DELTA SCUTI STAR AD CMI

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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来源期刊

Revista Mexicana de Astronomia y Astrofisica 地学天文-天文与天体物理

CiteScore

1.30

自引率

10.00%

发文量

审稿时长

>12 weeks

期刊介绍： The Revista Mexicana de Astronomía y Astrofísica, founded in 1974, publishes original research papers in all branches of astronomy, astrophysics and closely related fields. Two numbers per year are issued and are distributed free of charge to all institutions engaged in the fields covered by the RMxAA.