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http://hdl.handle.net/1959.3/190664 - Tidal disruption of the
Magellanic Clouds by the Milky Way - Putman, M. E.; Gibson, B.
K.; Staveley-Smith, L.; Banks, G.; Barnes, D. G.; Bhatal, R.;
Disney, M. J.; Ekers, R. D.; Freeman, K. C.; Haynes, R. F.;
Henning, P.; Jerjen, H.; Kilborn, V.; Koribalski, B.; Knezek,
P.; Malin, D. F.; Mould, J. R.; Oosterloo, T.; Price, R. M.;
Ryder, S. D.; Sadler, E. M.; Stewart, I.; Stootman, F.; Vaile,
R. A.; Webster, R. L.; Wright, A. E. - Interactions between
galaxies are common, and influence physical properties such as
the global morphology and star-formation rate1 (Hubble type).
Galaxies can interact in many different ways: they can merge
together; they can pass through each other, with gas being
stripped from the smaller of the two and compressed in the
larger; and they can interact gravitationally (including, for
exam