@article {24010,
	title = {Kinematics in the outer parts of the SMC.},
	volume = {261},
	year = {1993},
	month = {1993/04/1},
	pages = {873 - 882},
	abstract = {Extensive studies of red horizontal branch (clump) stars in the outer parts of the Small Magellanic Cloud (SMC) have suggested the presence of a large line-of-sight depth in the north-eastern region. A sample of red horizontal branch stars in the area of maximum depth was observed in 1989 December and 1990 December with the multi-object spectroscopic facility Autofib at the 3.9-m Anglo-Australian Telescope, with the purpose of deriving the velocity distribution for these stars. The data show a well- defined correlation between distance along the line of sight and radial velocity (corresponding to 8 km s^-1^ kpc^-1^), which may be interpreted as the result of the tidal interaction between the SMC and the LMC.},
	isbn = {0035-8711},
	url = {https://ui.adsabs.harvard.edu/abs/1993MNRAS.261..873H},
	author = {Hatzidimitriou, D. and Cannon, R. D. and Hawkins, M. R. S.}
}
