On the Force Associated with Absorption of Spectral Line Radiation
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This article is published in Monthly Notices of the Royal Astronomical Society.The article was published on 1974-11-01 and is currently open access. It has received 81 citations till now. The article focuses on the topics: Absorption (electromagnetic radiation) & Spectral line.read more
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Type Ia Supernovae: Influence of the Initial Composition on the Nucleosynthesis, Light Curves, and Spectra and Consequences for the Determination of ΩM and Λ
Peter Höflich,Peter Höflich,Peter Höflich,John C Wheeler,John C Wheeler,Friedrich-Karl Thielemann,Friedrich-Karl Thielemann +6 more
TL;DR: In this article, the influence of the initial composition of the exploding white dwarf on the nucleosynthesis, light curves, and spectra of Type Ia supernovae has been studied in order to evaluate the size of evolutionary effects on cosmological timescales, how the effects can be recognized, and how one may be able to correct for them.
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Spectroscopic Constraints on Models of Ion Cyclotron Resonance Heating in the Polar Solar Corona and High-Speed Solar Wind
TL;DR: In this paper, a theoretical model of the nonequilibrium plasma state of the polar solar corona is presented, where the primary energy deposition mechanism is the dissipation of high-frequency (10-10,000 Hz) ion cyclotron resonant Alfven waves.
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Ion Cyclotron Wave Dissipation in the Solar Corona: The Summed Effect of More than 2000 Ion Species
TL;DR: In this paper, the dissipation of ion cyclotron resonant Alfven waves in the extended solar corona is examined in detail, and the wave damping arising from more than 2000 low-abundance ion species is taken into account.
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Aspherical Explosion Models for SN 1998bw/GRB 980425
TL;DR: In this paper, the authors investigated the hypothesis that SNe Ic and SN 1998bw are the results of aspherical explosions along the rotational axis of basically spherical, non-degenerate C/O cores of massive stars.
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Line-driven Stellar Winds: The Dynamical Role of Diffuse Radiation Gradients and Limitations to the Sobolev Approach
Stanley P. Owocki,Joachim Puls +1 more
TL;DR: In this paper, a non-local escape-integral source function (EISF) method for computing the line force toward time-dependent simulations is applied. But the authors do not consider the role of the diffuse, scattered radiation field in the dynamics around the wind sonic point.