Marina Romanova

Marina Romanova
Marina Romanova
Alma mater	Moscow State University
	Scientific career
Fields	computational astrophysicics
Institutions	Russian Space Research Institute; Cornell University

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,^[1] and the formation of magnetic towers along the rotation axis of the accretion disks of black holes.^[2] She works as a senior research associate in the Cornell Center for Astrophysics and Planetary Science, in the Department of Astronomy at Cornell University.^[3]

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Marina Romanova
Alma mater	Moscow State University
Scientific career
Fields	computational astrophysicics
Institutions	Russian Space Research Institute Cornell University