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- W127204461 abstract "We use a simple, spherically symmetric model for the Galaxy based on the rotation curve for the inner parts. We extrapolate beyond the rotation curve boundary, assuming a dark corona whose total mass is a model parameter. For each mass value assume we calculate the allowed angular-momentum interval for which a cloud is neither tidally disrupted, nor escapes. On the basis of this investigation we reach a conclusion about the expected mass of the Galaxy." @default.
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- W127204461 date "1991-01-01" @default.
- W127204461 modified "2023-10-17" @default.
- W127204461 title "Orbits of the Magellanic Clouds" @default.
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- W127204461 doi "https://doi.org/10.1017/s0074180900201204" @default.
- W127204461 hasPublicationYear "1991" @default.
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