Results 251 to 260 of about 35,447 (292)

Nightside clouds and disequilibrium chemistry on the hot Jupiter WASP-43b. [PDF]

open access: yesNat Astron
Bell TJ   +82 more
europepmc   +1 more source

A hot white dwarf merger remnant revealed by an ultraviolet detection of carbon. [PDF]

open access: yesNat Astron
Sahu S   +9 more
europepmc   +1 more source

Accreting White Dwarfs: An Unreview. [PDF]

open access: yesSpace Sci Rev
Scaringi S, Knigge C, de Martino D.
europepmc   +1 more source

Opacity and radiative power losses calculations

High Energy Density Physics, 2009
In this contribution we present results on opacity and radiative power losses in laser-produced plasmas. We focus our attention on the inner shell transition array 1s-2p in an aluminum plasma. At high densities, electron, Doppler and ion Stark broadening play a role in line merging.
D Benredjem, A Calisti, C Mossé
exaly   +3 more sources

Calculations of the radiative opacity of laser-produced plasmas

Journal of Physics B: Atomic, Molecular and Optical Physics, 1992
The author presents a model for the calculation of the radiative opacity of high-power laser-produced plasmas in local thermodynamic equilibrium (LTE). The model uses detailed configuration accounting in an open shell for both the line and photoelectric absorption.
S J Rose
exaly   +2 more sources

The Effect of Degeneracy on the Scattering Contribution to the Radiative Opacity

Astrophysical Journal, 1995
The effect of partial free electron degeneracy on the scattering contribution to the radiative opacity is of interest in calculations of the structure and evolution of stars, particularly the Sun, where the plasma at the Sun's center is partially degenerate and scattering is a major contribution to the opacity.
S J Rose
exaly   +2 more sources

Opacity Project data on CD for mean opacities and radiative accelerations

Monthly Notices of the Royal Astronomical Society: Letters, 2005
M J Seaton
exaly   +2 more sources

Radiative opacities for stellar envelopes

Physica Scripta, 1995
Recent advances in the field of opacity calculations for stellar envelopes are summarized. The methods used and the results obtained in the last decade by two independent groups are discussed briefly. Some of the important effects of the new data on astrophysical studies are outlined.
openaire   +1 more source

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