压舱物 发表于 2025-4-1 01:55:09
Unified NLTE Model Atmospheres Including Spherical Extension and Stellar Winds: EUV — Fluxes and thee. The models are of spherical geometry and extended over the entire sub- and supersonic atmosphere. They need only stellar effective temperature, gravity, radius and helium abundance as free parameters and are in principle self-consistent. We have calculated a large grid of models for Central Stars有帮助 发表于 2025-4-1 07:56:26
Non-LTE Model Atmosphere Calculations with Approximate Lambda Operatorste lambda operators and a new numerical approach for the linearization procedure are presented..The optimum . approximate lambda operator was found by Olson & Kunasz (1987). An increase in convergence rate is only possible with . approximate lambda operators. The introduction of tridiagonal operatorBridle 发表于 2025-4-1 11:18:02
NLTE Model Atmospheres for Hot Starsre we present recent results of our NLTE model atmosphere calculations for hot sdO stars including very elaborate C IV, N IV and N V model ions simultaneously in order to determine the ../.. and ../.. abundance ratios.Mercantile 发表于 2025-4-1 14:49:55
http://reply.papertrans.cn/88/8772/877148/877148_64.pngBarter 发表于 2025-4-1 19:04:27
http://reply.papertrans.cn/88/8772/877148/877148_65.pngsquander 发表于 2025-4-1 23:07:19
Time-Dependent Two-Dimensional Radiation Hydrodynamics of Accreting Matter onto Highly Magnetized Neaccretion of matter onto the highly magnetized polar caps of luminous x-ray pulsars. The calculations show a structure in the accretion column very different from previous one-zone uniform models. We have included all the relevant magnetic field corrections to both the hydrodynamics and the radiativTOXIN 发表于 2025-4-2 06:34:29
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