Marina Romanova
Marina M. Romanova is a Russian-American computational astrophysicist, known for her work simulating the magnetohydrodynamics of accretion disks, including their interactions with the stellar magnetic fields of T Tauri stars and other young magnetized stars, and the formation of magnetic towers along the rotation axis of the accretion disks of black holes. She works as a senior research associate in the Cornell Center for Astrophysics and Planetary Science, in the Department of Astronomy at Cornell University. Provided by Wikipedia-
1by Vera Serga, Regina Burve, Aija Krumina, Marina Romanova, Eugene A. Kotomin, Anatoli I. PopovGet full text
Published 2021-04-01
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2by Liga AVOTINA, Elina PAJUSTE, Marina ROMANOVA, Gennady ENICHEK, Aleksandrs ZASLAVSKIS, Valentina KINERTE, Juris AVOTINS, Yuri DEHTJARS, Gunta KIZANEGet full text
Published 2019-11-01
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