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Double, triple and quadruple-line spectroscopic binary candidates within the Gaia-ESO Survey

Published online by Cambridge University Press:  07 March 2018

Thibault Merle
Affiliation:
Institut d'Astronomie et d'Astrophysique, Université Libre de Bruxelles CP 226, boulevard du Triomphe, B-1050 Brussels, Belgium email: thibault.merle@ulb.ac.be
Sophie Van Eck
Affiliation:
Institut d'Astronomie et d'Astrophysique, Université Libre de Bruxelles CP 226, boulevard du Triomphe, B-1050 Brussels, Belgium email: thibault.merle@ulb.ac.be
Alain Jorissen
Affiliation:
Institut d'Astronomie et d'Astrophysique, Université Libre de Bruxelles CP 226, boulevard du Triomphe, B-1050 Brussels, Belgium email: thibault.merle@ulb.ac.be
Mathieu Van der Swaelmen
Affiliation:
Institut d'Astronomie et d'Astrophysique, Université Libre de Bruxelles CP 226, boulevard du Triomphe, B-1050 Brussels, Belgium email: thibault.merle@ulb.ac.be
Gregor Traven
Affiliation:
Faculty of Mathematics and Physics, University of Ljubljana, Jadranska 19, 1000, Ljubljana, Slovenia
Tomaz Zwitter
Affiliation:
Faculty of Mathematics and Physics, University of Ljubljana, Jadranska 19, 1000, Ljubljana, Slovenia
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Abstract

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The Gaia-ESO Survey (GES, Gilmore et al. 2012) provides a unique opportunity to detect spectroscopically multiplicity among different populations of the Galaxy using the cross-correlation functions (CCFs). We present here the GES internal Data Release 4 (iDR4) results of the detection of double, triple and quadruple-line spectroscopic binary candidates (SBs) and discuss some peculiar systems.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2018 

References

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Merle, T., Van Eck, Jorissen A., Van der Swaelmen, M. et al. submitted to A&A Google Scholar
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