2 papers
astro-ph.SR2026
New possible way to determine stellar wind terminal velocity from analysis of Lyman- absorption spectra
Sergey D. Korolkov, Vladislav V. Izmodenov
Stellar winds interact with the partially ionized interstellar medium (ISM), forming astrospheres. A key feature of this interaction is the hydrogen wall - secondary interstellar a…
astro-ph.SR2025
Effects of angular scattering and H+p, H+H collisions on the properties of interstellar atoms in the heliosphere
A. V. Titova, V. V. Izmodenov, S. D. Korolkov
Interstellar hydrogen atoms (H atoms) penetrate into the heliosphere through the region of the solar wind interaction with the interstellar plasma due to their large mean free path…