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To the development of the mechanism of interaction of galactic comets with the terrestrial planets the physical processes at once. At that, with a decrease of power of gaseous envelope of planet, the action

To the development of the mechanism of interaction of galactic comets with the terrestrial planets the physical processes at once. At that, with a decrease of power of gaseous envelope of planet, the action

Overcoming the Limitations of the Energy-limited Approximation for Planet Atmospheric Escape-atmosphere hydrodynamic models computed for a wide range of planets with hydrogen-dominated atmospheres from which we

Close-in sub-Neptunes reveal the past rotation history of their host stars: atmospheric evolution of planets in the HD3167 and K2-32 planetary systemsPlanet atmospheric escape induced by high-energy stellar irradiation is a key phenomenon shaping

Modeling the Ly alpha transit absorption of the hot Jupiter HD 189733b absorption of neutral hydrogen has been observed in the Lyα line during transits of several close-in gaseous

Modeling the Lyα transit absorption of the hot Jupiter HD 189733b=Modeling the Ly alpha transit absorption of the hot Jupiter HD 189733b absorption of neutral hydrogen has been observed in the Lyα line during transits of several close-in gaseous

Effect of changes in gaseous environment and temperature on animals with diabetesIn contrast to normal environmental conditions (normal temperature and gaseous composition

Supermassive hot Jupiters provide more favourable conditions for the generation of radio emission via the cyclotron maser instability - a case study based on Tau Bootis b Tau Bootis b-like planets (a supermassive hot Jupiter with 5.84 Jupiter masses and 1.06 Jupiter radii

Novel position-sensitive gaseous detectors with solid photocathodesCurrently, a revolution is happening in the development of gaseous detectors of photons

Grid of upper atmosphere models for 1-40 M⊕ planets: application to CoRoT-7 b and HD 219134 b,c to produce a large grid of about 7000 models covering planets with masses 1-39 M⊕ with hydrogen

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