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TheGaia-ESO Survey: double-, triple-, and quadruple-line spectroscopic binary candidates

2017/07/06 by T. Merle, S. Van Eck, A. Jorissen +35 · 69 citations
Physics and Astronomy · #Astronomical spectroscopy #Astronomy and Astrophysical Research #Astrophysics and Star Formation Studies #Binary number #Binary star #Binary system #Distribution (mathematics) #Emission spectrum #Spectroscopy #Stellar, planetary, and galactic studies #astro-ph.SR

paper · pdf · doi:10.1051/0004-6361/201730442

published in Astronomy and Astrophysics 608, A95 (EDP Sciences) · 36 pages, 30 figures, 12 tables. Accepted for publication by A&A on 2017-07-05

arxiv created 2017/07/06 · openalex created_date 2017/07/14 · openalex publication_date 2017/07/28 · arxiv updated 2017/12/13 · openalex updated_date 2026/08/05

Abstract

Context. The Gaia-ESO Survey (GES) is a large spectroscopic survey that provides a unique opportunity to study the distribution of spectroscopic multiple systems among different populations of the Galaxy.

Citations

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