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- W61340710 abstract "We present evidence that the properties of the high-velocity cloud catalogued as #187 by Wakker & van Woerden (1991) (HVC287+22+240) can be explained if it is part of a leading arm counterpart of the Magellanic Stream, and we use this to argue that the HVC originated in the Magellanic Clouds after a tidal interaction." @default.
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- W61340710 date "1999-01-01" @default.
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- W61340710 title "The Metallicity and Dust Content of HVC287+22+240: Evidence for a Magellanic Clouds Origin" @default.
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- W61340710 doi "https://doi.org/10.1017/s0074180900118728" @default.
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