RESULTS OF OBSERVATIONS OF MAXIMA OF PULSATING STARS

被引：1

作者：

Pena, J. H. ^{[1
,2
,3
]}

Huepa, H. ^{[1
]}

Pina, D. S. ^{[2
,3
]}

Guillen, J.

Renteria, A. ^{[1
]}

Paredes, J. D. ^{[4
]}

Munoz, R. ^{[5
]}

Donaire, J. ^{[5
]}

Benadalid, T. ^{[5
]}

机构：

[1] Univ Nacl Autonoma Mexico, Observ Astron Nacl Tonantzintla, Mexico City, DF, Mexico

[2] Univ Nacl Autonoma Mexico, Inst Astron, Mexico City, DF, Mexico

[3] Univ Nacl Autonoma Mexico, Fac Ciencias, Mexico City, DF, Mexico

[4] Cent Univ Venezuela, Fac Ciencias, Caracas, Venezuela

[5] Univ Mayor San Andres, Planetario Max Schreier, La Paz, Bolivia

来源：

REVISTA MEXICANA DE ASTRONOMIA Y ASTROFISICA | 2021年 / 57卷 / 01期

关键词：

ephemerides; stars; variables; Scuti;

D O I：

10.22201/ia.01851101p.2021.57.01.18

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The systematic study of some HADS stars, recognized as variables for decades, has allowed us to provide data on their secular variations through O-C analysis. However, some of the data have large gaps without observations. This is our motivation for continuously observing these stars as part of the research carried out by the "Grupo de Astronomi ' a Observacional del Observatorio de Tonantzintla" (GAOOT). This article is our third compilation of times of maxima for pulsating stars. These observations have been carried out at the Observatorio Astrono ' mico Nacional de Tonantzintla (TNT) and San Pedro M ' artir (SPM), Me ' xico and for the first time we also present data from the Complejo Astrono ' mico de Cota Cota, Bolivia (Universidad Mayor de San Andre ' s) and the Observatorio Astrono ' mico Centroamericano de Suyapa, Honduras (Universidad Nacional Auto ' noma de Honduras).

引用

页码：241 / 246

页数：6

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