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Stars with expanding atmospheres
Vistas in Astronomy, 1956Abstract Most stars are stabilized spheres whose outer strata are nearly quiescent. Those exceptional objects in whose atmospheres outward motions have been observed may be placed in three groups: pulsating stars, stars with occasional outbursts, and stars with a continual outflow of atoms.
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Nucleosynthesis in neutron star atmospheres
Astrophysics and Space Science, 1969The composition of neutron star atmospheres is calculated as a function of time including effects of diffusion, cooling and thermonuclear reactions. A seven-component nuclear reaction network with includes He4, C12, O16, Ne20, Mg24, Si28 and Fe56 is utilized.
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Magnetized atoms in star atmospheres
AIP Conference Proceedings, 2000Magnetic white dwarfs possess strong magnetic fields which can vary in the wide range 100 T–105T. Atoms and molecules of their atmospheres which are exposed to such extreme fields severely change their electronic structure and properties. In order to understand the observed spectra of magnetic cosmic objects it is indispensable to perform detailed ...
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Hydrodynamical Model Atmospheres of Metal‐Poor Stars
AIP Conference Proceedings, 2008Standard one‐dimensional (1D) model atmospheres rely on the assumption of radiative equilibrium in the non‐convective part of the stellar photosphere. However, gas‐dynamical effects can lead to dramatic deviations from radiative equilibrium conditions, especially in metal‐poor stellar atmospheres.
Ludwig, Hans-Günter +4 more
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Atmospheres of Rocky Exoplanets
Annual Review of Astronomy and Astrophysics, 2022Robin D Wordsworth, Laura Kreidberg
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Dynamics and clouds in planetary atmospheres from telescopic observations
Astronomy and Astrophysics Review, 2023Agustin Maria Sanchez Lavega +1 more
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The Roar of the Crowd: How Interaction Ritual Chains Create Social Atmospheres
Journal of Marketing, 2022Tim Hill +2 more
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Atmospheres of nonrotating baryon stars
Astrophysics, 1974G. S. Saakyan, D. M. Sedrakyan
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