"galaxies evolution; galaxies interaction; kinematics and dynamics; Magellanic Cculds; methods: N-body simulations"@en . "Pohyb Magellanov\u00FDch oblak\u016F v prostoru: jsou slapov\u00E9 modely vylou\u010Deny?"@cs . . . "691" . . . . . "Palou\u0161, Jan" . . "Nov\u00E9 hodnoty vlastn\u00EDch pohyb\u016F Velk\u00E9ho a Mal\u00E9ho Magellanova oblaku odvozen\u00E9 Kallivazalil et al. odhaluj\u00ED neo\u010Dek\u00E1van\u011B rychl\u00FD prostorov\u00FD pohyb Magellanova syst\u00E9mu. To m\u016F\u017Ee znamenat, \u017Ee se oblaka p\u0159ibli\u017Euj\u00ED k Ml\u00E9\u010Dn\u00E9 dr\u00E1ze poprv\u00E9, co\u017E znemo\u017E\u0148uje interpretaci tvaru a rychlost\u00ED HI v Magellanov\u011B proudu, mostu a ve vedouc\u00EDm rameni pomoc\u00ED model\u016F pou\u017Eivaj\u00EDc\u00EDch slapov\u00E9 s\u00EDly."@cs . "Astrophysical Journal" . . "2"^^ . . "[40788974B75F]" . "2" . "Theis, Ch." . "P(KJB300030801), P(LC06014), Z(AV0Z10030501)" . . "9"^^ . . "US - Spojen\u00E9 st\u00E1ty americk\u00E9" . "3"^^ . "Spatial motion of the Magellanic clouds: tidal models rulled out?" . "Pohyb Magellanov\u00FDch oblak\u016F v prostoru: jsou slapov\u00E9 modely vylou\u010Deny?"@cs . "Spatial motion of the Magellanic clouds: tidal models rulled out?"@en . . "Recently, Kallivayalil et al. derived new values of the proper motion for the Large and Small Magellanic Clouds (LMC and SMC, respectively). The spatial velocities of both Clouds are unexpectedly higher than their previous values resulting from agreement between the available theoretical models of the Magellanic System and the observations of neutral hydrogen (H I) associated with the LMC and the SMC. We investigated this hypothesis for the pure tidal models, as they were the first ones devised to explain the evolution of the Magellanic System, and the tidal stripping is intrinsically involved in every model assuming the gravitational interaction." . "342743" . . . "R\u016F\u017Ei\u010Dka, Adam" . . . "Recently, Kallivayalil et al. derived new values of the proper motion for the Large and Small Magellanic Clouds (LMC and SMC, respectively). The spatial velocities of both Clouds are unexpectedly higher than their previous values resulting from agreement between the available theoretical models of the Magellanic System and the observations of neutral hydrogen (H I) associated with the LMC and the SMC. We investigated this hypothesis for the pure tidal models, as they were the first ones devised to explain the evolution of the Magellanic System, and the tidal stripping is intrinsically involved in every model assuming the gravitational interaction."@en . "Spatial motion of the Magellanic clouds: tidal models rulled out?"@en . . "Spatial motion of the Magellanic clouds: tidal models rulled out?" . . . "RIV/67985815:_____/09:00322209" . "0004-637X" . . "RIV/67985815:_____/09:00322209!RIV09-AV0-67985815" . . "263304300072" .