RR Lyrae Search and Stellar Populations Study in Canis Major: Preliminary Results

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Autor principal: C. E. Mateu
Formato: Artículo científico
Lenguaje:en
Publicado: Universidad Nacional Autónoma de México 2006
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author C. E. Mateu
author_facet C. E. Mateu
contents RR Lyrae Search and Stellar Populations Study in Canis Major: Preliminary Results C. E. Mateu L. Miller A. K. Vivas R. Zinn Física, Astronomía y Matemáticas GALAXY: FORMATION GALAXY: STRUCTURE GALAXIES: INTERACTIONS STARS: VARIABLES: OTHER We present preliminary results of a RR Lyrae star search and stellar populations study performed in the Canis Major overdensity, spanning an area of 8:35 sq deg. The observations were made in R and V bands, with the QUEST camera installed in the 1-m Jürgen Stock Telescope at the Venezuela National Observatory. The resulting Hess diagram shows a possible, but weak, red giant branch and no obvious horizontal branch, red clump or main sequence turnoff. After a multi{epoch photometric search, 6 RR Lyrae stars were confirmed with further observations obtained at the 1.0-m and 1.3-m telescopes of the SMARTS consortium at CTIO. From these confirmed RR Lyrae stars, ve of them have heliocentric distances between 5 and 7 kpc. Confirmation of their physical association with the Canis Major system awaits for a study of their radial velocities. 2006 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57102509 en http://www.redalyc.org/revista.oa?id=571 Revista Mexicana de Astronomía y Astrofísica application/pdf Universidad Nacional Autónoma de México Revista Mexicana de Astronomía y Astrofísica (México) Vol.25
format Artículo científico
id redalyc_57102509
institution Redalyc
language en
publishDate 2006
publisher Universidad Nacional Autónoma de México
spellingShingle RR Lyrae Search and Stellar Populations Study in Canis Major: Preliminary Results
C. E. Mateu
Física, Astronomía y Matemáticas
GALAXY: FORMATION
GALAXY: STRUCTURE
GALAXIES: INTERACTIONS
STARS: VARIABLES: OTHER
RR Lyrae Search and Stellar Populations Study in Canis Major: Preliminary Results C. E. Mateu L. Miller A. K. Vivas R. Zinn Física, Astronomía y Matemáticas GALAXY: FORMATION GALAXY: STRUCTURE GALAXIES: INTERACTIONS STARS: VARIABLES: OTHER We present preliminary results of a RR Lyrae star search and stellar populations study performed in the Canis Major overdensity, spanning an area of 8:35 sq deg. The observations were made in R and V bands, with the QUEST camera installed in the 1-m Jürgen Stock Telescope at the Venezuela National Observatory. The resulting Hess diagram shows a possible, but weak, red giant branch and no obvious horizontal branch, red clump or main sequence turnoff. After a multi{epoch photometric search, 6 RR Lyrae stars were confirmed with further observations obtained at the 1.0-m and 1.3-m telescopes of the SMARTS consortium at CTIO. From these confirmed RR Lyrae stars, ve of them have heliocentric distances between 5 and 7 kpc. Confirmation of their physical association with the Canis Major system awaits for a study of their radial velocities. 2006 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57102509 en http://www.redalyc.org/revista.oa?id=571 Revista Mexicana de Astronomía y Astrofísica application/pdf Universidad Nacional Autónoma de México Revista Mexicana de Astronomía y Astrofísica (México) Vol.25
title RR Lyrae Search and Stellar Populations Study in Canis Major: Preliminary Results
topic Física, Astronomía y Matemáticas
GALAXY: FORMATION
GALAXY: STRUCTURE
GALAXIES: INTERACTIONS
STARS: VARIABLES: OTHER
url https://www.redalyc.org/articulo.oa?id=57102509