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- W3166405501 abstract "The Magellanic System includes some of the nearest examples of galaxies disturbed by galaxy interactions. These interactions have redistributed much of their gas into the halos of the Milky Way (MW) and the Magellanic Clouds. We present Wisconsin Hα Mapper kinematically resolved observations of the warm ionized gas in the Magellanic Bridge over the velocity range of +100 to +300 km s −1 in the local standard of rest reference frame. These observations include the first full Hα intensity map and the corresponding intensity-weighted mean velocity map of the Magellanic Bridge across (l,b) = (281. 5, −30. 0) to (302. 5, −46. ◦ 7). Using the Hα emission from the Small Magellanic Cloud (SMC)-Tail and the Bridge, we estimate that the mass of the ionized material is between 0" @default.
- W3166405501 created "2021-06-22" @default.
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- W3166405501 date "2013-01-01" @default.
- W3166405501 modified "2023-10-16" @default.
- W3166405501 title "Warm, Ionized Gas Revealed in the Magellanic Bridge Tidal Remnant: Constraining the Baryon Content and the Escaping Ionizing Photons around Dwarf Galaxies" @default.
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- W3166405501 hasPublicationYear "2013" @default.
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