0124848 - ASU-R 20010101 RIV US eng C - Konferenční příspěvek (zahraniční konf.)
Šimon, Vojtěch
Activity of the dwarf nova CH UMa.
X-ray astronomy. Stellar endpoints, AGN, and the diffuse background. Melville: American Institute of Physics, 2001 - (White, N.; Malaguti, G.; Palumbo, G.), s. 947-950
[X-ray astronomy. Stellar endpoints, AGN, and the diffuse background. Bologna (IT), 06.09.1999-10.09.1999]
Grant CEP: GA MŠMT ME 137
Výzkumný záměr: CEZ:AV0Z1003909
Klíčová slova: stars * activity * circumstellar matter * novae * cataclysmic variables
Kód oboru RIV: BN - Astronomie a nebeská mechanika, astrofyzika

The outbursts in CH UMa can be divided into two classes (bright and faint). The maximum brightness of the outbursts tends to decrease over 25 years. The bright outbursts fall into two subtypes according to their decay branches. The recurrence time of the bright outbursts 300-370 days displays variations with a strong secular trend.
Trvalý link: http://hdl.handle.net/11104/0023107