Metallicity and distance of NGC 6362 from its RR Lyrae and SX Phoenicis stars

Author:

Arellano Ferro A.1,Ahumada J. A.2,Bustos Fierro I. H.2,Calderón J. H.23,Morrell N. I.4

Affiliation:

1. Instituto de AstronomíaUniversidad Nacional Autónoma de México Ciudad de México Mexico

2. Observatorio AstronómicoUniversidad Nacional de Córdoba Córdoba Argentina

3. Consejo Nacional de Investigaciones Científicas y Técnicas (CONICET) Córdoba Argentina

4. Las Campanas ObservatoryCarnegie Observatories La Serena Chile

Funder

Universidad Nacional Autónoma de México

Publisher

Wiley

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 7 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. Isochrone fitting of Galactic globular clusters – IV. NGC 6362 and NGC 6723;Monthly Notices of the Royal Astronomical Society;2022-11-12

2. A VINDICATION OF THE RR LYRAE FOURIER LIGHT CURVE DECOMPOSITION FOR THE CALCULATION OF METALLICITY AND DISTANCE IN GLOBULAR CLUSTERS;Revista Mexicana de Astronomía y Astrofísica;2022-10-01

3. NGC 1261: A TIME-SERIES VI STUDY OF ITS VARIABLE STARS;Revista Mexicana de Astronomía y Astrofísica;2019-09-13

4. Gaia parallax of Milky Way globular clusters – A solution of mixture model;Monthly Notices of the Royal Astronomical Society;2019-08-21

5. Extraction of globular clusters members with Gaia DR2 astrometry;Monthly Notices of the Royal Astronomical Society;2019-07-10

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