000006662 001__ 6662
000006662 005__ 20240125125157.0
000006662 0247_ $$2DOI$$a10.48550/arXiv.2311.09764
000006662 037__ $$aSCART-2024-0040
000006662 100__ $$aMerle, T.
000006662 245__ $$aDancing with the stars: a review on stellar multiplicity 
000006662 260__ $$c2023
000006662 520__ $$aStars like company. They are mostly formed in clusters and their lives are often altered by the presence of one or more companions. Interaction processes between components may lead to complex outcomes like Algols, blue stragglers, chemically altered stars, type Ia supernovae, as well as progenitors of gravitational wave sources, to cite a few. Observational astronomy has entered the era of big data, and thanks to large surveys like spatial missions Kepler, TESS, Gaia, and ground-based spectroscopic surveys like RAVE, Gaia-ESO, APOGEE, LAMOST, GALAH (to name a few) the field is going through a true revolution, as illustrated by the recent detection of stellar black holes and neutron stars as companions of massive but also low-mass stars. In this review, I will present why it is important to care about stellar multiples, what are the main large surveys in which many binaries are harvested, and finally present some features related to the largest catalogue of astrometric, spectroscopic and eclipsing binaries provided by the Non-Single Star catalogue of Gaia, which is, to date, the largest homogeneous catalogue of stellar binaries. 
000006662 536__ $$aPrf-2020-033_BISTRO/$$cPrf-2020-033_BISTRO/$$fPrf-2020-033_BISTRO
000006662 594__ $$aNO
000006662 6531_ $$abinary stars
000006662 6531_ $$astellar multiplicity
000006662 6531_ $$aspectroscopic binaries
000006662 6531_ $$aeclipsing binaries
000006662 6531_ $$aastrometric binaries
000006662 773__ $$pBulletin de la Société Royale des Sciences de Liège$$y2023
000006662 8560_ $$fthibault.merle@ksb-orb.be
000006662 85642 $$ahttps://ui.adsabs.harvard.edu/abs/2023arXiv231109764M/abstract
000006662 905__ $$aaccepted to be published in
000006662 980__ $$aREFERD