Simpson, Jeffrey DMartell, SarahDa Costa, GaryHorner, JonathanWyse, Rosemary F GTing, Yuan-SenAsplund, MartinBland-Hawthorn, JossBuder, SvenDe Silva, Gayandhi MFreeman, KennethKos, J.Lewis, GeraintLind, K.Sharma, SanjibNordlander, Thomas2023-01-182023-01-180035-8711http://hdl.handle.net/1885/283836Using kinematics from Gaia and the large elemental abundance space of the second data release of the GALAH survey, we identify two new members of the Fimbulthul stellar stream, and chemically tag them to massive, multimetallic globular cluster ω Centauri. Recent analysis of the second data release of Gaia had revealed the Fimbulthul stellar stream in the halo of the Milky Way. It had been proposed that the stream is associated with the ω Cen, but this proposition relied exclusively upon the kinematics and metallicities of the stars to make the association. In this work, we find our two new members of the stream to be metal-poor stars that are enhanced in sodium and aluminium, typical of second population globular cluster stars, but not otherwise seen in field stars. Furthermore, the stars share the s-process abundance pattern seen in ω Cen, which is rare in field stars. Apart from one star within 1.5 deg of ω Cen, we find no other stars observed by GALAH spatially near ω Cen or the Fimbulthul stream that could be kinematically and chemically linked to the cluster. Chemically tagging stars in the Fimbulthul stream to ω Cen confirms the earlier work, and further links this tidal feature in the Milky Way halo to ω Cen.Parts of this research were conducted by the Australian Research Council Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D), through project number CE170100013. JDS, SLM, and DZ acknowledge the support of the Australian Research Council through Discovery Project grant DP180101791. SB acknowledges funds from the Alexander von Humboldt Foundation in the framework of the Sofja Kovalevskaja Award endowed by the Federal Ministry of Education and Research. TZ acknowledge the financial support from the Slovenian Research Agency (research core funding No. P1-0188). KF and Y-ST are grateful for support from Australian Research Council grant DP160103747. Y-ST is grateful to be supported by the NASA Hubble Fellowship grant HST-HF2-51425.001 awarded by the Space Telescope Science Institute.application/pdfen-AU© 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Societyglobular clusters: individual: ω Cengalaxy: halogalaxy: kinematics and dynamics202010.1093/mnras/stz31052021-11-28