La estrella variable BZ
UMa está en Outburst observaciones CCD son necesarias
Imagen CCD Enero 16- 2005
Algunas observaciones:
BZ UMA 20050116.9229 11.40
GZN
GZN:Alfredo Glez-Herrera
RZD:Diego Rodriguez
EJC: José Castillo Escudero
SQU: Joaquín Sánchez López
MM: Manuel Méndez.
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Variable Star BZ UMa
Outburst of BZ UMa (25 February
2004)
BZ UMa was discovered by Markaryan (Astrofizika
4, 144) on one of his
objective prism plates. The star was bright (10.5mag pg) on one exposure and faint (16mag) at other dates. One further maximum (11.0mag vis.) has been observed since,by members of the AAVSO (Mayall, Journ. R. Astr. Soc. Canada 66, 181).IBVS 2256 |
Outburst report was by Michael Simonsen,
(MI. USA) mag 11.6 on 2004 Feb 25.29. According to the AAVSO International
Database, BZ UMa appears to be in outburst, its first since December,2002.
BZ UMa is classified as a UG by the GCVS. However, it is suggested to be a SU UMa subtype due to its short orbital period and mass ratio (Jurcevic et. al. PASP 05/1994). According to W. WENZEL , BZ UMa might be an intermediate object in connecting the U Gem and WZ Sge classes. (IBVS 2256) Observations. BZ UMA FEB 27.8507 2453063.3507 13.71 RZD CCDV BZ UMA FEB 28.7889 2453064.2889 14.80 CGY CCD Diego Rodriguez=RZD
Toni Climet Garcia= CGY
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