" mass-loss" . "The results of the project enrich the information base of fundamental research in radiation transfer and properties of astrophysical objects. The outputs were primarily published in 18 articles in impact journals, 14 proceedings contributions and 4 book chapters. The project proceeded without flaws in compliance with methodological and financial rules. The panel evaluated the project as excellent."@en . . "2012-03-30+02:00"^^ . "stellar" . . . . . . "V\u00FDsledky projektu obohacuj\u00ED informa\u010Dn\u00ED b\u00E1zi z\u00E1kladn\u00EDho v\u00FDzkumu v oblasti p\u0159enosu z\u00E1\u0159en\u00ED i vlastnost\u00ED astrofyzik\u00E1ln\u00EDch objekt\u016F. V\u00FDstupy byly publikov\u00E1ny p\u0159edev\u0161\u00EDm v 18 \u010Dl\u00E1nc\u00EDch v impaktov\u00FDch \u010Dasopisech, ale i ve 14 sborn\u00EDkov\u00FDch p\u0159\u00EDsp\u011Bvc\u00EDch a 4 kni\u017En\u00EDch kapitol\u00E1ch. \u0158e\u0161en\u00ED prob\u00EDhalo bez nedostatk\u016F v dodr\u017Eov\u00E1n\u00ED metodick\u00FDch a finan\u010Dn\u00EDch pravidel. Celkov\u011B panel projekt hodnot\u00ED jako vynikaj\u00EDc\u00ED."@cs . "34"^^ . " rate" . . "34"^^ . . "http://www.isvav.cz/projectDetail.do?rowId=GA205/08/0003"^^ . . . . . "GA205/08/0003" . "Hmotn\u00E9 hork\u00E9 hv\u011Bzdy tvo\u0159\u00ED d\u016Fle\u017Eitou slo\u017Eku jak na\u0161\u00ED Galaxie, tak i mnoh\u00FDch dal\u0161\u00EDch galaxi\u00ED. Proto je znalost jejich v\u00FDvoje a jejich vlivu na okolohv\u011Bzdn\u00E9 prost\u0159ed\u00ED nezbytn\u00E1 pro pochopen\u00ED struktury a v\u00FDvoje jednotliv\u00FDch galaxi\u00ED. Jedn\u00EDm z nejpal\u010Div\u011Bji\u0161\u00EDch s" . "2008-01-01+01:00"^^ . "P\u0159edpov\u011Bdi rychlosti ztr\u00E1ty hmoty hork\u00FDch hv\u011Bzd" . . . . "0"^^ . "Mass-loss rate predictions for hot stars"@en . "2014-01-30+01:00"^^ . "2012-12-31+01:00"^^ . . "1"^^ . "stellar; wind; mass-loss; rate; hydrodynamics"@en . "1"^^ . . "Massive hot stars constitute an important part of our Galaxy and many other galaxies. Consequently, a detailed knowledge of their evolution and of their influence on the circumstellar environment is necessary for our understanding of the structure and e"@en . " wind" . .