| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 1779405 | New Astronomy | 2012 | 5 Pages |
Abstract
⺠We detected the optical oscillation with a period of 3.238 h in the cataclysmic variable V378 Peg. ⺠This oscillation is unstable both in amplitude and in phase with random phase changes within 10-20% of the period. ⺠Because of its instability we attribute this oscillation to superhumps. ⺠V378 Peg shows no outburst typical of dwarf novae and appears as a nova-like variable. ⺠Hence, the detected superhumps are permanent superhumps, but not common superhumps observed in SU UMa stars.
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Authors
V.P. Kozhevnikov,