Mimoradny seminar AsU

Vazeni studenti a mili kolegove,
V tomto obtiznem case pozvolna koncicich prazdnin a dovolenych, dovoluji siVas pozvat na seminar a diskuzi se zahranicnimi hosty. Tema seminare patrido oblasti vysokofrekvencnich oscilaci rentgenoveho zareni, ktere sepozoruji u nekolika desitek neutronovych hvezd a cernych der vedvojhvezdnych soustavach. Pricina oscilaci neni znama (o hypotezy nouzeneni), a tak jde o docela zajimave tema. Prednasejicijsou zajimave osobnosti a zname celebrity tohoto oboru. Bude prilezitostposlechnout si dve prednasky (jedna pozorovatelska, jedna teoreticka) anavazat neformalnimi otazkami a diskuzi. Neobvykly termin a misto (sobota, Narodni 3) jsou dany snahou dostatvsechny cizince, zabyvajici se ruznymi aspekty tohoto tematu, do jednemistnosti soucasne. Patrne se zucastni rovnez dalsi zahranicnihoste s pravdepodobnosti v intervalu (0,1). Neobvykly termin a misto ovsem velmi zneklidnuji organizatora seminaru.Doufam, ze studenti a kolegove, kteri se mohou zucastnit, me nenechaji vsale samotneho s presilovkou prednasejicich. Prosim take o rozsireni tetopozvanky mezi dalsi zajemce ve Vasem okoli.

--Additional information follows.The first compelling evidence of a large mass function in an X-raytransient was discovered by Ron Remillard and Jeff McClintock (then at MIT)in 1985. For a number of years this source was one of a kind. In 1992 twomore such sources were identified, one of them by McClintock and Remillardin collaboration. Recently, both authors have significantly contributedto the effort of redefining the states of active accretion in compactbinaries. Shoji Kato has pioneered the whole subject of discoseismology.He is a co-author of an influentional book on accretion discs and theiroscillations. http://arxiv.org/abs/astro-ph/0306213 http://arxiv.org/abs/astro-ph/0409051