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Collision strengths for nebular [O iii] optical and infrared lines

Monthly notices of the Royal Astronomical Society, 2014-07, Vol.441 (4), p.3028-3039

2014

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Helium line emissivities for nebular astrophysics

Monthly notices of the Royal Astronomical Society, 2022-04, Vol.513 (1), p.1198-1209

2022

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Electron-impact excitation of O ii fine-structure levels

Monthly notices of the Royal Astronomical Society, 2009-08, Vol.397 (2), p.903-912

2009

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Collision strengths and transition probabilities for Co iii forbidden lines

Monthly notices of the Royal Astronomical Society, 2016-07, Vol.459 (3), p.2558-2565

2016

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Collision strengths and transition probabilities for Co ii infrared forbidden lines

Monthly notices of the Royal Astronomical Society, 2016-02, Vol.456 (2), p.1974-1981

2016

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Effective collision strengths for excitation and de-excitation of nebular [O iii] optical and infrared lines with κ distributed electron energies

Monthly notices of the Royal Astronomical Society, 2015-05, Vol.449 (3), p.2974-2979

2015

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MOCASSIN: a fully three-dimensional Monte Carlo photoionization code

Monthly notices of the Royal Astronomical Society, 2003-04, Vol.340 (4), p.1136-1152

2003

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Erratum: 'Improved He i emissivities in the Case B approximation'

Monthly notices of the Royal Astronomical Society. Letters, 2013-07, Vol.433 (1), p.L89-L90

2013

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Theoretical values for the [O iii] 5007/4959 line-intensity ratio and homologous cases

Monthly notices of the Royal Astronomical Society, 2000-03, Vol.312 (4), p.813-816

2000

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The dusty mocassin: fully self-consistent 3D photoionization and dust radiative transfer models

Monthly notices of the Royal Astronomical Society, 2005-09, Vol.362 (3), p.1038-1046

2005

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Recombination coefficients for O ii lines in nebular conditions

Monthly notices of the Royal Astronomical Society, 2017-09, Vol.470 (1), p.379-389

2017

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Theoretical calculations of the H i, He i and He ii free–bound continuous emission spectra

Monthly notices of the Royal Astronomical Society, 2006-11, Vol.372 (4), p.1875-1878

2006

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A deep survey of heavy element lines in planetary nebulae - II. Recombination-line abundances and evidence for cold plasma

Monthly notices of the Royal Astronomical Society, 2004-09, Vol.353 (3), p.953-979

2004

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On the validity of the ICFT R-matrix method: Fe xiv

Monthly notices of the Royal Astronomical Society, 2015-12, Vol.454 (3), p.2909-2917

2015

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Plasma diagnostics for planetary nebulae and H ii regions using the N ii and O ii optical recombination lines

Monthly notices of the Royal Astronomical Society, 2013-02, Vol.428 (4), p.3443-3461

2013

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Chemical abundances for Hf 2-2, a planetary nebula with the strongest-known heavy-element recombination lines

Monthly notices of the Royal Astronomical Society, 2006-06, Vol.368 (4), p.1959-1970

2006

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Electron temperatures and densities of planetary nebulae determined from the nebular hydrogen recombination spectrum and temperature and density variations

Monthly notices of the Royal Astronomical Society, 2004-07, Vol.351 (3), p.935-955

2004

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Improved Optimization Strategy for Irradiance Equalization in Dynamic Photovoltaic Arrays

IEEE transactions on power electronics, 2013-06, Vol.28 (6), p.2946-2956

2013

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The hydrogen-deficient knot of the ‘born-again’ planetary nebula Abell 58 (V605 Aql)

Monthly notices of the Royal Astronomical Society, 2008-02, Vol.383 (4), p.1639-1648

2008

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Modelling low charge ions in the solar atmosphere

Monthly notices of the Royal Astronomical Society, 2021-08, Vol.505 (3), p.3968-3981

2021

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New atomic data for C i Rydberg states compared with solar UV spectra

Monthly notices of the Royal Astronomical Society, 2023-11, Vol.526 (1), p.1396-1407

2023

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Heavy elements in Galactic and Magellanic Cloud H ii regions: recombination-line versus forbidden-line abundances

Monthly notices of the Royal Astronomical Society, 2003-01, Vol.338 (3), p.687-710

2003

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Improved He i emissivities in the case B approximation

Monthly notices of the Royal Astronomical Society. Letters, 2012-09, Vol.425 (1), p.L28-L31

2012

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NGC 6153: a super-metal-rich planetary nebula?

Monthly notices of the Royal Astronomical Society, 2000-03, Vol.312 (3), p.585-628

2000

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The continuum emission spectrum of Hf 2-2 near the Balmer limit and the ORL versus CEL abundance and temperature discrepancy

Monthly notices of the Royal Astronomical Society, 2014-05, Vol.440 (3), p.2581-2587

2014

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Collision strengths for nebular [O iii] optical and infrared lines

Helium line emissivities for nebular astrophysics

Electron-impact excitation of O ii fine-structure levels

Collision strengths and transition probabilities for Co iii forbidden lines

Collision strengths and transition probabilities for Co ii infrared forbidden lines

Effective collision strengths for excitation and de-excitation of nebular [O iii] optical and infrared lines with κ distributed electron energies

MOCASSIN: a fully three-dimensional Monte Carlo photoionization code

Erratum: 'Improved He i emissivities in the Case B approximation'

Theoretical values for the [O iii] 5007/4959 line-intensity ratio and homologous cases

The dusty mocassin: fully self-consistent 3D photoionization and dust radiative transfer models

Recombination coefficients for O ii lines in nebular conditions

Theoretical calculations of the H i, He i and He ii free–bound continuous emission spectra

A deep survey of heavy element lines in planetary nebulae - II. Recombination-line abundances and evidence for cold plasma

On the validity of the ICFT R-matrix method: Fe xiv

Plasma diagnostics for planetary nebulae and H ii regions using the N ii and O ii optical recombination lines

Chemical abundances for Hf 2-2, a planetary nebula with the strongest-known heavy-element recombination lines

Electron temperatures and densities of planetary nebulae determined from the nebular hydrogen recombination spectrum and temperature and density variations

Improved Optimization Strategy for Irradiance Equalization in Dynamic Photovoltaic Arrays

The hydrogen-deficient knot of the ‘born-again’ planetary nebula Abell 58 (V605 Aql)

Modelling low charge ions in the solar atmosphere

New atomic data for C i Rydberg states compared with solar UV spectra

Heavy elements in Galactic and Magellanic Cloud H ii regions: recombination-line versus forbidden-line abundances

Improved He i emissivities in the case B approximation

NGC 6153: a super-metal-rich planetary nebula?

The continuum emission spectrum of Hf 2-2 near the Balmer limit and the ORL versus CEL abundance and temperature discrepancy

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