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Интеллектуальная Система Тематического Исследования НАукометрических данных |
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The behaviour of V392 Per is similar to Recurrent Nova U Sco and very fast nova V2672 Oph, suspected RN. All three objects displayed a He/N spectrum classification, large expansion velocities and triple peaked emission-line profiles during the decline. Morpho-kinematic modelling of V2672 Oph and V392 Per suggest that the systems are seen nearly pole-on.