ИСТИНА |
Войти в систему Регистрация |
|
ИСТИНА ИНХС РАН |
||
We analyse UBVRcIc light curves of the classical Novae V2467 Cyg and V2468 Cyg in time interval from their outbursts till now. The light of both stars faded by 8 mag. The stars show outburst activity with cycles 21.3d (V2467 Cyg) and 2.4d (V2468 Cyg). From our multicolor phorometry we determined absolute magnitudes in outburst.