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Identification of binary and multiple systems in TGAS using the Virtual Observatory

Published online by Cambridge University Press:  07 March 2018

F. Jiménez-Esteban  and
E. Solano
F. Jiménez-Esteban
Affiliation:
Centro de Astrobiología (INTA-CSIC), Madrid, Spain email: fran.jimenez-esteban@cab.inta-csic.es Spanish Virtual Observatory Suffolk University
E. Solano
Affiliation:
Centro de Astrobiología (INTA-CSIC), Madrid, Spain email: fran.jimenez-esteban@cab.inta-csic.es Spanish Virtual Observatory
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Abstract

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Binary and multiple stars have long provided an effective method of testing stellar formation and evolution theories. In particular, wide binary systems with separations > 20,000 au are particularly challenging as their physical separations are beyond the typical size of a collapsing cloud core (5,000 - 10,000 au). We present here a preliminary work in which we make use of the TGAS catalogue and Virtual Observatory tools and services (Aladin, TOPCAT, STILTS, VOSA, VizieR) to identify binary and multiple star candidate systems. The catalogue will be available from the Spanish VO portal (http://svo.cab.inta-csic.es) in the coming months.

Keywords

Astronomical data basescataloguesvirtual observatory toolsparallaxesproper motionsbinaries: visual
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 12 , Symposium S330: Astrometry and Astrophysics in the Gaia sky , April 2017 , pp. 225 - 226
Copyright
Copyright © International Astronomical Union 2018 

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