LEADER 02458nam0 2200505 i 450 001 VAN0132852 005 20230621114625.345 017 70$2N$a9783319036502 100 $a20210329d2014 |0itac50 ba 101 $aeng 102 $aCH 105 $a|||| ||||| 200 1 $aSymmetries and Dynamics of Star Clusters$eDoctoral Thesis accepted by the Charles University in Prague, Czech Republic$fJaroslav Haas 210 $aCham$cSpringer$d2014 215 $axvi, 79 p.$cill.$d24 cm 410 1$1001VAN0104193$12001 $aSpringer theses$erecognizing outstanding Ph.D. research$1210 $aBerlin$cSpringer$d2010- 500 1$3VAN0134831$aSymmetries and Dynamics of Star Clusters$91770398 606 $a00A79 (77-XX)$xPhysics [MSC 2020]$3VANC023182$2MF 606 $a85-XX$xAstronomy and Astrophysics [MSC 2020]$3VANC023246$2MF 606 $a85A15$xGalactic and stellar structure [MSC 2020]$3VANC023268$2MF 606 $a83C57$xBlack holes [MSC 2020]$3VANC023271$2MF 606 $a85A05$xGalactic and stellar dynamics [MSC 2020]$3VANC036147$2MF 606 $a83C22$xEinstein-Maxwell equations [MSC 2020]$3VANC036148$2MF 606 $a83C25$xApproximation procedures, weak fields in general relativity and gravitational theory [MSC 2020]$3VANC036149$2MF 610 $aDynamics of Star Clusters$9KW:K 610 $aFeeding of supermassive black holes$9KW:K 610 $aGalactic Center$9KW:K 610 $aGalactic Centre$9KW:K 610 $aGalactic Nucleus$9KW:K 610 $aModelling Nuclear Star Clusters$9KW:K 610 $aNumerical N-body Modelling$9KW:K 610 $aOrbital Evolution of Star Clusters$9KW:K 610 $aStellar Disc Around Supermassive Black Hole$9KW:K 610 $aSymmetries of Star Clusters$9KW:K 620 $aCH$dCham$3VANL001889 700 1$aHaas$bJaroslav$3VANV106691$0791795 712 $aSpringer $3VANV108073$4650 801 $aIT$bSOL$c20240614$gRICA 856 4 $uhttp://doi.org/10.1007/978-3-319-03650-2$zE-book ? Accesso al full-text attraverso riconoscimento IP di Ateneo, proxy e/o Shibboleth 899 $aBIBLIOTECA DEL DIPARTIMENTO DI MATEMATICA E FISICA$1IT-CE0120$2VAN08 912 $fN 912 $aVAN0132852 950 $aBIBLIOTECA DEL DIPARTIMENTO DI MATEMATICA E FISICA$d08CONS e-book 2030 $e08eMF2030 20210329 996 $aSymmetries and Dynamics of Star Clusters$91770398 997 $aUNICAMPANIA