VVV IR HIGH PROPER MOTION STARS

Fuente: Redalyc
Guardado en:
Detalles Bibliográficos
Autor principal: R. Kurtev
Formato: Artículo científico
Lenguaje:en
Publicado: Universidad Nacional Autónoma de México 2015
Materias:
Acceso en línea:
Etiquetas: Agregar Etiqueta
Sin Etiquetas, Sea el primero en etiquetar este registro!
_version_ 1876471620514611200
author R. Kurtev
author_facet R. Kurtev
contents VVV IR HIGH PROPER MOTION STARS R. Kurtev M. Gromadzki J.C. Beamin K. Peña S. Folkes V.D. Ivanov J. Borissova M. Kuhn V. Villanueva D. Minniti R. Mendez P. Lucas L. Smith D. Pinfield A. Antonova Física, Astronomía y Matemáticas low mass Stars surveys proper motions We used the VISTA Variables en V ́ıa L ́actea (VVV) survey to search for large proper motion (PM) objects in the zone of avoidance in the Milky Way bulge and southern Galactic disk. This s urvey is multi-epoch and already spans a period of more than four years, giving us an excellent opportunit y for proper motion and parallax studies. We found around 1700 PM objects with PM > 30 mas yr − 1 . The majority of them are early and mid M-dwarfs. There are also few later spectral type objects, as well as numerous new K- and G-dwarfs. 75 of the stars have PM > 300 mas − 1 and 189 stars have PM > 200 mas − 1 . There are only 42 previously known stars in the VVV area with proper motion PM > 200 mas − 1 . We also found three dM+WD binaries and new members of the immediate solar vicinity of 25 pc. We generated a catalog which will be a complementary to the existing catalogs outside this zone. 2015 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57150514013 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.46
format Artículo científico
id redalyc_57150514013
institution Redalyc
language en
publishDate 2015
publisher Universidad Nacional Autónoma de México
spellingShingle VVV IR HIGH PROPER MOTION STARS
R. Kurtev
Física, Astronomía y Matemáticas
low
mass
Stars
surveys
proper motions
VVV IR HIGH PROPER MOTION STARS R. Kurtev M. Gromadzki J.C. Beamin K. Peña S. Folkes V.D. Ivanov J. Borissova M. Kuhn V. Villanueva D. Minniti R. Mendez P. Lucas L. Smith D. Pinfield A. Antonova Física, Astronomía y Matemáticas low mass Stars surveys proper motions We used the VISTA Variables en V ́ıa L ́actea (VVV) survey to search for large proper motion (PM) objects in the zone of avoidance in the Milky Way bulge and southern Galactic disk. This s urvey is multi-epoch and already spans a period of more than four years, giving us an excellent opportunit y for proper motion and parallax studies. We found around 1700 PM objects with PM > 30 mas yr − 1 . The majority of them are early and mid M-dwarfs. There are also few later spectral type objects, as well as numerous new K- and G-dwarfs. 75 of the stars have PM > 300 mas − 1 and 189 stars have PM > 200 mas − 1 . There are only 42 previously known stars in the VVV area with proper motion PM > 200 mas − 1 . We also found three dM+WD binaries and new members of the immediate solar vicinity of 25 pc. We generated a catalog which will be a complementary to the existing catalogs outside this zone. 2015 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57150514013 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.46
title VVV IR HIGH PROPER MOTION STARS
topic Física, Astronomía y Matemáticas
low
mass
Stars
surveys
proper motions
url https://www.redalyc.org/articulo.oa?id=57150514013