Activity of the dwarf nova CH UMa

Number of the records: 1

SYSNO ASEP	0124848
Document Type	C - Proceedings Paper (int. conf.)
R&D Document Type	Conference Paper
Title	Activity of the dwarf nova CH UMa
Author(s)	Šimon, Vojtěch (ASU-R)_{ORCID, RID}
Source Title	X-ray astronomy. Stellar endpoints, AGN, and the diffuse background / White N.E. ; Malaguti G. ; Palumbo G.. - Melville : American Institute of Physics, 2001
Pages	s. 947-950
Number of pages	4 s.
Action	X-ray astronomy. Stellar endpoints, AGN, and the diffuse background
Event date	06.09.1999-10.09.1999
VEvent location	Bologna
Country	IT - Italy
Event type	WRD
Language	eng - English
Country	US - United States
Keywords	stars ; activity ; circumstellar matter ; novae ; cataclysmic variables
Subject RIV	BN - Astronomy, Celestial Mechanics, Astrophysics
R&D Projects	ME 137 GA MŠMT - Ministry of Education, Youth and Sports (MEYS)
CEZ	AV0Z1003909 - ASU-R
Annotation	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.
Workplace	Astronomical Institute
Contact	Anežka Melichárková, bibl@asu.cas.cz, Tel.: 323 620 326
Year of Publishing	2002

Number of the records: 1