Variable Star WUMa

CROSS IDENTIFICATION: W UMa

W UMa = ADS 07494 = AN 1903.0003 = BD +56 1400 = HD 083950 = SAO 027364 

GCVS result

ID: 830006
Variable star: W UMa
RA 2000: 094345.5
DE 2000: +555709
RA 1950:
DE 1950:
Type of variability: EW/KW
Max (mag): 7.75
Min (mag): 8.48
Photometric system: V
Epoch (JD): 45765.7385
Period (d): 0.33363749
Year of outburst for N, SN:
M-m (or D):
Spectrum: F8Vp+F8Vp
Study reference: 00001
Chart or phot. ref.: 00462
Cases of non-existence:

GCVS NOTE result

"ADS 7494 A (B 12.35m, 6.5"", 44deg, 1963)." "dI = 0.037P Soft X-ray source. LX/Lbol = 1.7*10**(-4). P var. Min I = 2420980.8093 + 0.333638880d*E "(JD2416000 - 21000) "0.333636993d*E (JD2421000 - 33000) [01760] Min I = 2435918.4169 + 0.33363832d*E (JD2433000 - 41000) "[05327] including depths of minima, var. A moving wave with Delta(m) = 0.025m y and P ~1100d [10067] was noted. A flare (Delta(m) = 1.5m, lambda 3300 A, delta(lambda) = 50 A, JD2438511.7, delta(t) = 7 min) was announced [05788]. The system contains gaseous streams, dark spots on the surface of the components. H and K CaII emission.

GCVS NOTES fulltext search:  

NSV: Suspected Variable NSV  not found.

BRKA result

Variable star: W UMa
Brightness type: 08
Points: 1
RA 2000: 094345.4
DE 2000: +555710
Max (mag): 7.75
Min (mag): 8.48
Sec (mag): 8.43
Photometric system: V
Epoch (JD): 51268.7233
Period (d): 0.33363808
D (hour): W
d (hour): 0.3
Astrophysical note: P1-2
Reference: IBVS 4752
Finding chart: K3

BRKA result

Variable star: W:UMa
Brightness type: 08
Points: 1
RA 2000: 094345.4
DE 2000: +555710
Max (mag): 7.75
Min (mag): 8.48
Sec (mag): 8.43
Photometric system: V
Epoch (JD): 51268.8901
Period (d): 0.33363808
D (hour): W
d (hour): 0.2
Astrophysical note:
Reference: Vyp
Finding chart: K3

MEKA: Variable star W 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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