seminar

1) Speaker: E.S. Kalinicheva Title: “Study of the evolution of exoplanet atmospheres” Abstract: see Russian version 2) Speaker: L.A. Maksimova Title: “Influence of Convective Instability and Self-Shading Effects on the Structure and Evolution of a Protoplanetary Disk” Abstract: see Russian version 3) Speaker: O.L. Ryabukhina Title: “A study of molecular filaments in star-forming region” Abstract:

The seminar will be held in a mixed format 1) Speaker: M.D. Sizova (INASAN) Title: “Kinematics of stellar streams, clusters and their decay products with Gaia data” Abstract: see Russian version Sign up for the seminar

The seminar will be held in a mixed format 1) Speaker: S.A. Drozdov (ASC LPI) Title: “IR and submm emission features of the inner regions of galaxies” Abstract: see Russian version Sign up for the seminar

The seminar will be held online 1) Speaker: K.I. Smirnova (UrFU) Title: “Star formation regions in normal and peculiar galaxies” Abstract: see Russian version

The seminar will be held in a mixed format 1) Speaker: A.F. Zakharov (ITEP, JINR) Title: “Shadows in the vicinity of the Galactic Center and in M87* as new tests of general relativity” Abstract: see Russian version Sign up for the seminar

The seminar will be held in a mixed format 1) Speaker: I.I. Baliukin (IKI RAS) Title: “Specific features of neutral component distribution in the heliosphere and the Earth’s exosphere” Abstract: see Russian version

The seminar will be held in a mixed format 1) Speaker: G.S. Fedoseev (UrFU) Title: “Laboratory investigations revealing solid-state formation routes of carbon- and nitrogen-bearing species in cold and low-density regions of space” Abstract: see Russian version

The seminar will be held in a mixed format 1) Speaker: A.V. Tutukov (INASAN) Title: “Evolution of planets, stars, galaxies, and their systems” Abstract: see Russian version

The seminar will be held in a mixed format 1) Speaker: M.V. Barkov (INASAN) Title: “Fast radio bursts by high-frequency synchrotron maser emission generated at the reverse shock of a powerful magnetar flare” Abstract: We consider a magnetar flare model for fast radio bursts (FRBs). We show that millisecond burst of sufficient power can be