VVV IR high proper motion stars
link https://repositorio.uc.cl/handle/11534/84552account_box Kurtev, R.account_box Gromadzki, M.account_box Beamin Muhlenbrock, Juan Carlosaccount_box Pena, K.account_box Folkes, S.account_box Ivanov, V. D.account_box Borissova, J.account_box Kuhn, M.account_box Villanueva, V.account_box Minniti, D.account_box Mendez, R.account_box Lucas, P.account_box Smith, L.account_box Pinfield, D.account_box Antonova, A.account_box Vieira, Kaccount_box VanAltena, Waccount_box Mendez, RA
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We used the VISTA Variables en Via Lactea (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 survey is multi-epoch and already spans a period of more than four years, giving us an excellent opportunity 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.
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| Autor | Kurtev, R. Gromadzki, M. Beamin Muhlenbrock, Juan Carlos Pena, K. Folkes, S. Ivanov, V. D. Borissova, J. Kuhn, M. Villanueva, V. Minniti, D. Mendez, R. Lucas, P. Smith, L. Pinfield, D. Antonova, A. Vieira, K VanAltena, W Mendez, RA |
| Título | VVV IR high proper motion stars |
| Revista | RevMexAA (Serie de Conferencias) |
| ISSN | 1405-2059 |
| Volumen | 46 |
| Página inicio | 50 |
| Página final | 55 |
| Fecha de publicación | 2015 |
| Resumen | We used the VISTA Variables en Via Lactea (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 survey is multi-epoch and already spans a period of more than four years, giving us an excellent opportunity 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. |
| Derechos | acceso restringido |
| Editorial | UNIVERSIDAD NACIONAL AUTONOMA MEXICO INSTITUTO ASTRONOMIA |
| Enlace | |
| Id de publicación en WoS | WOS:000371549500012 |
| Palabra clave | infrared: stars proper motions stars: low-mass surveys SOLAR NEIGHBORHOOD MULTIPLICITY CATALOG |
| Se encuentra en | 6th Scientific Meeting on Dynamical Astronomy in Latin America (ADeLA 2014), SEP 29-OCT 01, 2014, Santiago, CHILE |
| Tema ODS | 11 Sustainable Cities and Communities |
| Tema ODS español | 11 Ciudades y comunidades sostenibles |
| Temática | Astronomía |
| Tipo de documento | comunicación de congreso |