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We report the discovery of 24 spectroscopic binary companions to giant stars. We fully constrain the orbital solution for 6 of these systems. We cannot unambiguously derive the orbital elements for the remaining stars because the phase coverage is incomplete. Of these stars, 6 present radial velo...


Bluhm, PJones, MIVanzi, LSoto, MGVoss, JWittenmyer, RADrass, HJenkins, JSOlivares, FMennickent, REVuckovic, MRojo, PMelo, CHF[New spectroscopic binary companions of giant stars and updated metallicity distribution for binary systems]New spectroscopic binary companions of giant stars and updated metallicity distribution for binary systems

Fernandez-Trincado, JGRobin, ACMoreno, ESchiavon, RPPerez, AEGVieira, KCunha, KZamora, OSneden, CSouto, DCarrera, RJohnson, JAShetrone, MZasowski, GGarcia-Hernandez, DAMajewski, SRReyle, CBlanco-Cuaresma, SMartinez-Medina, LAPerez-Villegas, AValenzuela, OPichardo, BMeza, AMeszaros, SSobeck, JGeisler, DAnders, FSchultheis, MTang, BRoman-Lopes, AMennickent, REPan, KNitschelm, CAllard, F[DISCOVERY OF A METAL-POOR FIELD GIANT WITH A GLOBULAR CLUSTER SECOND-GENERATION ABUNDANCE PATTERN]DISCOVERY OF A METAL-POOR FIELD GIANT WITH A GLOBULAR CLUSTER SECOND-GENERATION ABUNDANCE PATTERN

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