Luisi, MatteoAnderson, L.D.Bania, Thomas M.Balser, Dana S.Wenger, Trey V.Kepley, Amanda A.2024-05-092024-05-092018-08M. Luisi, L.D. Anderson, T.M. Bania, D.S. Balser, T.V. Wenger, A.A. Kepley. 2018. "Hydrogen Radio Recombination Line Emission from M51 and NGC 628" Publications of the Astronomical Society of the Pacific, Volume 130, Issue 990, pp.084101-084101. https://doi.org/10.1088/1538-3873/aac8e90004-62801538-3873https://hdl.handle.net/2144/48726We report the discovery of hydrogen radio recombination line (RRL) emission from two galaxies with star formation rates (SFRs) similar to that of the Milky Way: M51 and NGC628. We use the Green Bank Telescope (GBT) to measure ∼15 Hnɑ recombination transitions simultaneously and average these data to improve our spectral signal-to-noise ratio. We show that our data can be used to estimate the total ionizing photon flux of these two sources, and we derive their SFRs within the GBT beam: Ψ_OB = 3.46 M⊙ yr^-1 for M51 and Ψ_OB = 0.56 M⊙ yr^-1 for NGC628. Here, we demonstrate that it is possible to detect RRLs from normal galaxies that are not undergoing a starburst with current instrumentation and reasonable integration times (∼12 hr for each source). We also show that we can characterize the overall star-forming properties of M51 and NGC628, although the GBT beam cannot resolve individual HII region complexes. Our results suggest that future instruments, such as the Square Kilometre Array and the Next Generation Very Large Array, will be able to detect RRL emission from a multitude of Milky Way-like galaxies, making it possible to determine SFRs of normal galaxies unaffected by extinction and to measure global star formation properties in the local universe.p. 084101enScience & technologyPhysical sciencesAstronomy & astrophysicsGalaxies: individual (M51, NGC 628, M100, M101, NGC 3184)Galaxies: ISMRadio lines: galaxiesRadio lines: ISMIonized gasNearby galaxiesStar-formationHIContinuumDensityRegionsProjectAtlasAstronomical and space sciencesAstronomical sciencesParticle and high energy physicsAstrophysics of galaxiesArticle2024-02-1810.1088/1538-3873/aac8e90000-0003-4866-460X (Bania, TM)389697