Variable Star RWTri


CROSS IDENTIFICATION: RW Tri

RW Tri = AN 1938.0005 


GCVS result

ID: 800015
Variable star: RW Tri
RA 2000: 022536.2
DE 2000: +280551
RA 1950:
DE 1950:
Type of variability: EA/WD+NL
Max (mag): 12.50
Min (mag): 15.61
Photometric system: V
Epoch (JD): 43512.6615
Period (d): 0.231883276
Year of outburst for N, SN:
M-m (or D): 07
Spectrum: pec(cont+e)+M0V
Study reference: 00001
Chart or phot. ref.: 09472
Cases of non-existence:


GCVS NOTE result

The depth of Min I 1.12m - 2.21m. D = 0.052P - 0.086P, d ~0.03P. P var? [03434, 09858, 9859]. Strong fluctuations of light outside eclipses. the lower the brightness outside the eclipse, the deeper the Min. In J, K light Min II of 0.16m J depth was found at the phase 0.50P [10053]. Flat spectrum of the accretion disc with emission lines.

GCVS NOTES fulltext search:  


NSV: Suspected Variable NSV  not found.


BRKA result

Variable star: RW Tri
Brightness type: 14
Points: 5
RA 2000: 022536.6
DE 2000: +280548
Max (mag): 12.50
Min (mag): 15.61
Sec (mag):
Photometric system: V
Epoch (JD): 43512.6615
Period (d): 0.231883276
D (hour): 0.4
d (hour): 0.2
Astrophysical note: P1?K2E3-4
Reference: GCVSe2001
Finding chart: K1

MEKA: Variable star RW Tri 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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