<?xml version="1.0" encoding="UTF-8"?><xml><records><record><source-app name="Biblio" version="7.x">Drupal-Biblio</source-app><ref-type>17</ref-type><contributors><authors><author><style face="normal" font="default" size="100%">Hatzidimitriou, D.</style></author><author><style face="normal" font="default" size="100%">Cannon, R. D.</style></author><author><style face="normal" font="default" size="100%">Hawkins, M. R. S.</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">Kinematics in the outer parts of the SMC.</style></title><short-title><style face="normal" font="default" size="100%">Monthly Notices of the Royal Astronomical Society</style></short-title></titles><dates><year><style  face="normal" font="default" size="100%">1993</style></year><pub-dates><date><style  face="normal" font="default" size="100%">1993/04/1</style></date></pub-dates></dates><urls><web-urls><url><style face="normal" font="default" size="100%">https://ui.adsabs.harvard.edu/abs/1993MNRAS.261..873H</style></url></web-urls></urls><volume><style face="normal" font="default" size="100%">261</style></volume><pages><style face="normal" font="default" size="100%">873 - 882</style></pages><isbn><style face="normal" font="default" size="100%">0035-8711</style></isbn><language><style face="normal" font="default" size="100%">eng</style></language><abstract><style face="normal" font="default" size="100%">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.</style></abstract></record></records></xml>