Fu, Sal WanyingSal WanyingFuSimon, Joshua D.Joshua D.SimonShetrone, MatthewMatthewShetroneBovy, JoJoBovyBeers, Timothy C.Timothy C.BeersFernandez-Trincado, J. G.J. G.Fernandez-TrincadoPlacco, Vinicius M.Vinicius M.PlaccoZamora, OlgaOlgaZamoraAllende Prieto, CarlosCarlosAllende PrietoGarcia-Hernandez, D. A.D. A.Garcia-HernandezHarding, PaulPaulHardingIvans, IneseIneseIvansLane, RichardRichardLaneNitschelm, ChristianChristianNitschelmRoman-Lopes, AlexandreAlexandreRoman-LopesSobeck, JenniferJenniferSobeck2025-12-302025-12-3020181538-4357https://hdl.handle.net/20.500.12740/24099We present a search for new members of the 300 km s(-1) stream (300S) near the dwarf galaxy Segue 1 using wide-field survey data. We identify 11 previously unknown bright stream members in the APOGEE-2 and SEGUE-1 and 2 spectroscopic surveys. Based on the spatial distribution of the high-velocity stars, we confirm for the first time that this kinematic structure is associated with a 24 degrees-long stream seen in SDSS and Pan-STARRS imaging data. The 300S stars display a metallicity range of -2.17 < [Fe/H] < -1.24, with an intrinsic dispersion of 0.21(-0.09)(+0.12)dex. They also have chemical abundance patterns similar to those of Local Group dwarf galaxies, as well as that of the Milky Way halo. Using the open-source code galpy to model the orbit of the stream, we find that the progenitor of the stream passed perigalacticon about 70 Myr ago, with a closest approach to the Galactic center of about 4.1 kpc. Using Pan-STARRS DR1 data, we obtain an integrated stream luminosity of 4 x 10(3) L-circle dot . We conclude that the progenitor of the stream was a dwarf galaxy that is probably similar to the satellites that were accreted to build the present-day Milky Way halo.Acceso Abiertogalaxies: dwarfGalaxy: haloGalaxy: structurestars: kinematics and dynamicshttp://dx.doi.org/10.3847/1538-4357/aad9f9