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We attempt to identify RR Lyrae (RRL) stars in stellar streams that mighthave escaped from seven globular clusters (GCs) based on proper motions,distances, color-magnitude diagrams, and other properties extracted from theGaia Early Data Release 3 (EDR3) database. Specifically, we cross-match twolarge RRL stars catalogs (from Gaia DR2 and Catalina Sky Survey) with eachother and with the EDR3 database and we end up with a sample of ~ 150,000unique RRL stars. We calculate distances to RRL stars using the (M_G-[Fe/H])and (M_V-[Fe/H]) absolute magnitude-metallicity relations and adopt [Fe/H]values for the GCs from different spectroscopic studies. We also constrain oursearch in areas where stellar streams associated with GCs were previouslysuggested or identified in other studies. We identify 24 RRL stars that mighthave escaped from the following seven GCs: Palomar 13 (Pal 13), NGC 6341 (M92),NGC 5904 (M5), NGC 5466, NGC 1261, NGC 288, and NGC 1851. We list our findingsin Table 2.

RR Lyrae Stars In Stellar Streams with Gaia: The Escapers