Variable Star BEUMa

CROSS IDENTIFICATION: BE UMa

BE UMa = PG 1155+492 = SVS 1424 

GCVS result

ID: 830083
Variable star: BE UMa
RA 2000: 115744.8
DE 2000: +485618
RA 1950:
DE 1950:
Type of variability: EA/D/WD
Max (mag): 14.8
Min (mag): 17.8
Photometric system: B
Epoch (JD): 44998.2809
Period (d): 2.2911665
Year of outburst for N, SN:
M-m (or D): 02
Spectrum: DO+MVe
Study reference: 09889
Chart or phot. ref.: 09875
Cases of non-existence:

GCVS NOTE result

d = 0.006P. Outside eclipses var 14.8m <= B <= 16.0m (reflection effect). The depth of eclipses for lambda lambda 3330 - 3700 A is greater than 4.3m,that for lambda lambda 5265 - 6005 A is 1.5m.

GCVS NOTES fulltext search:  

NSV: Suspected Variable NSV  not found.

BRKA result

Variable star: BE UMa
Brightness type: H16
Points: 10
RA 2000: 115744.9
DE 2000: +485618
Max (mag): 14.8
Min (mag): 17.8
Sec (mag):
Photometric system: B
Epoch (JD): 44998.2809
Period (d): 2.2911665
D (hour): 1.1
d (hour):
Astrophysical note:
Reference: GCVSe2001
Finding chart:

MEKA: Variable star BE UMa not found.

Please put the variable's designation into field in common style - for example: ZUMa, zuma, V477Cyg, v1182Cyg, NSV 255, nsv2544. Designation of bright variable stars like Beta Persei type in short style (three letters) - bet Per. The complete cross-identification among more then 30 catalogues will be done after submitting.
Spaces and cases are ingnored..


 
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