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ИСТИНА ЦЭМИ РАН |
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There will be presented the results of a detailed study of the starforming clumps in the gas ring of a nearby galaxy NGC 4324. The study is based on the data obtained with an imaging instrument MaNGaL - a narrowband tunable filter - developed in the SAO RAS. The gas inflow could be a source of a fresh star formation burst in a lenticular galaxy.