"GA202/97/0326" . . "The monitoring of the emission profiles of Balmer H-alfa line and some Fe II and Si II lines formed in the circumstellar emission disks of the Be-type stars has been carried out with the Ond\u0159ejov 2-m telescope since 1993 and should continue till completion of the here proposed grant. The monitoring was and will be completed by observations from the Haute Province, Calar Alto and ESO La Silla observatories. The preliminary results show that the project maximally uses scapabilities sof the Ond\u0159ejov telescope and represents an ideal program for it. The monitoring covering the period 1993-99 will provide us with an extraordinary data set in the given field. I order to derive the structure and evolution of the circumstellar disks, we will apply a high-quality modelling, which includes a three-dimensional radiative transfer calculations in emission lines coming from the circumstellar disks and tests of the model of the global oscillations in the disks. The physical and geometrical parameters of the disks w"@en . . "9"^^ . . "9"^^ . . . "V\u00FDsledky projektu p\u0159edstavuj\u00ED v\u00FDznamn\u00FD p\u0159\u00EDsp\u011Bvek, a to na sv\u011Btov\u00E9 \u00FArovni, k teoreticko-modelov\u00E9mu i observa\u010Dn\u00EDmu studiu vlastnost\u00ED, struktury a formov\u00E1n\u00ED cirkumstel\u00E1rn\u00EDch disk\u016F hv\u011Bzd typu Be. Ve spolupr\u00E1ci se zahrani\u010Dn\u00EDmi odborn\u00EDky byly nov\u00FDm zp\u016Fsobem vy"@cs . . . . . "Struktura a evoluce cirkumstel\u00E1rn\u00EDch emisn\u00EDch disk\u016F hv\u011Bzd typu Be" . . "Structure and evolution of the circumstellar emission disks of Be stars"@en . "http://www.isvav.cz/projectDetail.do?rowId=GA202/97/0326"^^ . "0"^^ . . "Monitorov\u00E1n\u00ED emisn\u00EDch profil\u016F Balmerovy \u010D\u00E1ry H-alfa a n\u011Bkter\u00FDch \u010Dar FeII a SiII, kter\u00E9 vznikaj\u00ED v cirkumstel\u00E1rn\u00EDch emisn\u00EDch disc\u00EDch hv\u011Bzd typu Be, prob\u00EDh\u00E1 za pomoci ond\u0159ejovsk\u00E9ho 2m dalekohledu od r.1993 a m\u011Blo by pokra\u010Dovat do ukon\u010Den\u00ED navrhovan\u00E9ho grantu. Monitoriv\u00E1n\u00ED bylo a bude dopl\u0148ov\u00E1no pozorov\u00E1n\u00EDmi z obsarvato\u0159\u00ED Haute Provence, Calar Alto a La Silla. P\u0159edb\u011B\u017En\u00E9 v\u00FDsledky ukazuj\u00ED, \u017Ee projekt vyu\u017E\u00EDv\u00E1 maxim\u00E1ln\u011B p\u0159ednosti ond\u0159ejovsk\u00E9ho dalekohledu a p\u0159edstavuje pro n\u011Bj ide\u00E1ln\u00ED program. Monitorov\u00E1n\u00ED prokr\u00FDvaj\u00EDc\u00ED obdob\u00ED 1993-99 poskytne vyj\u00EDme\u010Dn\u00FD pozorovac\u00ED soubor v dan\u00E9 oblasti v\u00FDzkumu. Vysoce kvalitn\u00ED modelov\u00E1n\u00ED pozorovac\u00EDch dat, kter\u00E9 zahrnuje t\u0159\u00EDrozm\u011Brn\u00E9 v\u00FDpo\u010Dty p\u0159enosu z\u00E1\u0159en\u00ED v emisn\u00EDch \u010Dar\u00E1ch vznikaj\u00EDc\u00EDch v okolohv\u011Bzdn\u00FDch disc\u00EDch a testy modelu glob\u00E1ln\u00EDch oscilac\u00ED v disc\u00EDch, bude pou\u017Eito s c\u00EDlem odvodit strukturu disk\u016F a jejich v\u00FDvoj. Fyzik\u00E1ln\u00ED a geometrick\u00E9 parametry disk\u016F budou nalezeny porovn\u00E1n\u00EDm pozorovan\u00FDch emisn\u00EDch profil\u016F s profily vypo\u010Dten\u00FDmi a modelov\u00E1n\u00EDm dynamick\u00FDch proces\u016F v disc\u00EDch. V" . . "0"^^ . . "1"^^ . .