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Details for Revision 1
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| Name |
V0373 Cas |
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| AAVSO UID |
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| Constellation |
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| J2000.0 |
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| B1950.0 |
23 53 02.66 +57 08 02.1 |
| Galactic coord. |
115.437 -4.644 |
Other names
(Internal only)
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AAVSO 2350+56 |
ALS 13294 |
BD+56 3115 |
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GSC 04009-00987 |
HD 224151 |
HIP 117957 |
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HR 9052 |
Hilt 1244 |
IRAS 23530+5707 |
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LS I +57 1 |
MCW 1140 |
PPM 42361 |
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SAO 35899 |
TYC 4009-987-1 |
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| Variability type |
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E:/GS |
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| Spectral type |
B0.5II+B0.5II |
| Mag. range |
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5.9 - 6.3 V |
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| Discoverer |
-- |
| Epoch |
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| Outburst |
-- |
| Period |
13.4192 d |
| Rise/eclipse dur. |
-- |
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Remarks
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Some references may be clicked to view in new window. Roll over index number to view submission details.
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1 |
Otero, Sebastian Alberto
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Non-eclipsing system. |
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2 |
GCVS Team |
An unique close binary. Porb = 13.4192d [D.G.Monet, ApJ 237, 513, 1980.]. Epoch of Min I is given close to the epoch of one of conjunctions. Min II - Min I = 0.58P. Maxima are very sharp. Max - Min II = 0.25P. It is not excluded that the star is an eclipsing one with physical variability of components, but eclipses, if they exist, cause only a very small part of the observed light variations. Range of light variations is given according to [E.Kollnig-Schattschneider, AN 271, 85, 1940.]. As a rule the amplitude is close to 0.1m. |
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References
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External Links
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Location
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Supporting Documents
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Revision History
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Currently approved revision is checked. Click revision number to view details of that revision.
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