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- W33390639 abstract "Tidal interaction models for the origin of the Magellanic Stream have been fairly successful in reproducing the radial velocities of the Stream (Lin and Lynden-Bell 1977, Davies and Wright 1977). However, no investigator has yet attained a self consistent treatment in which (1) the LMC and SMC are bound for at least 5×10 9 yr, (2) the passing Magellanic Clouds warp the galactic plane, and (3) the Stream velocities are reproduced (Fujimoto and Sofue 1977). Also, Mathewson, Schwarz, and Murray (1977) argue that their 21 cm observations are evidence against the tidal model. To avoid these problems, they suggest that the Magellanic Clouds pass through a hot coronal gas and produce vortices in their wake which radiatively cool to form the HI clouds comprising the Stream." @default.
- W33390639 created "2016-06-24" @default.
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- W33390639 date "1979-01-01" @default.
- W33390639 modified "2023-09-23" @default.
- W33390639 title "The galactic wake model of the Magellanic Stream" @default.
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- W33390639 doi "https://doi.org/10.1017/s0074180900015114" @default.
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