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Atomic data for opacity calculations. II. Computational methods

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TLDR
A detailed description of the methods being used in a collaborative effort which is referred to as the Opacity Project is given in this article, where the close-coupling approximation of electron-atom collision theory is used to calculate energies and wavefunctions for bound states, oscillator strengths, photoionisation cross sections and parameters for line broadening by electron impact.
Abstract
For pt.I see ibid., vol.20, p.6363-78 (1987). A general description of the data requirements for opacity calculations has been given in paper I. The present paper gives a detailed description of the methods being used in a collaborative effort which is referred to as the Opacity Project. The close-coupling approximation of electron-atom collision theory is used to calculate energies and wavefunctions for bound states, oscillator strengths, photoionisation cross sections and parameters for line broadening by electron impact. The computations are made using the R-matrix method together with new codes for calculating outer-region solutions and dipole integrals. Use of these techniques provides an efficient means of calculating large amounts of accurate atomic data.

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RMATRX1: Belfast atomic R-matrix codes

TL;DR: RMATRX1 as mentioned in this paper is a general program to calculate atomic continuum processes using the R -matrix method, including electronatom and electron-ion scattering, and radiative processes such as bound-bound transitions, photoionization and polarizabilities.
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ExoMol: molecular line lists for exoplanet and other atmospheres

TL;DR: The ExoMol project as discussed by the authors provides spectroscopic data on all the molecular transitions of importance in the atmospheres of exoplanets, which can be used for studies on cool stars, brown dwarfs and circumstellar environments.
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NGC 6153: a super-metal-rich planetary nebula?

TL;DR: In this article, the authors obtained deep optical spectra of the planetary nebula NGC 6153, both along its minor axis and by uniformly scanning a long slit across the whole nebula.
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X-ray reflected spectra from accretion disk models. I. Constant density atmospheres

TL;DR: In this paper, the effects of incident X-rays on the surface of an accretion disk by simultaneously solving the equations of radiative transfer, energy balance, and ionization equilibrium over a large range of column densities were considered.
Journal ArticleDOI

Photoionization of atoms using synchrotron radiation

TL;DR: A comprehensive review of photoionization of rare gas atoms using monochromatized synchrotron radiation is given in this paper, with a focus on the general experimental and theoretical background.
References
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Journal ArticleDOI

Quantum defect theory

TL;DR: Quantum defect theory (QDT) as mentioned in this paper is a unified theory of bound states, including series perturbations, autoionisation and electron-ion scattering, both elastic and inelastic.
Journal ArticleDOI

Techniques for the calculation of atomic structures and radiative data including relativistic corrections

TL;DR: Superstructure as mentioned in this paper is a general-purpose automatic atomic-structure program that uses multi-configuration type expansions to calculate term energies, intermediate-coupling energy levels, term coupling coefficients, and cascade coefficients.
Journal ArticleDOI

Atomic data for opacity calculations. I. General description

M. J. Seaton
- 14 Dec 1987 - 
TL;DR: In this paper, the authors give some of the formulae from thermodynamics and atomic physics which are required for opacity calculations, which are used to obtain improved values for opacities in stellar envelopes.
Journal ArticleDOI

Electron scattering by complex atoms

TL;DR: In this paper, a theory of electron scattering by complex atoms is developed in which the target atomic eigenstates and pseudostates are written as linear sums of configurations and the incident electron wave function is expanded in terms of orbitals which satisfy logarithmic boundary conditions on the surface of a sphere.
Journal ArticleDOI

On a screening theory of atomic spectra

TL;DR: In this article, a theoretical scheme for describing atomic spectra is developed, which differs from the current one in three main ways: (i) the nuclear charge Z enters explicitly into all predictions made with the new scheme, and (ii) certain effects of configuration interaction are allowed for in the first approximation.
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