Astronomy and Astrophysics – Astronomy
Scientist
Astronomy and Astrophysics
Astronomy
Scientist
Department of Applied Mathematics and Theoretical Physics, The Queen's University of Belfast, Belfast BT7 1NN, UK
School of Mathematics and Physics, The Queens University of Belfast, Belfast BT7 1NN, Northern Ireland, UK
Department of Applied Mathematics and Theoretical Physics, The Queen's University of Belfast, Belfast BT7 1NN
Department of Applied Mathematics and Theoretical Physics, The Queen's University of Belfast, Belfast BT7 1NN, Northern Ireland
Department of Applied Mathematics & Theoretical Physics, The Queen's University of Belfast, Belfast BT7 1NN, UK
School of Mathematics and Physics, The Queen's University of Belfast, Belfast BT7 1NN, Northern Ireland, UK
School of Mathematics and Physics, Queen's University Belfast, BT7 1NN, UK
Department of Applied Mathematics & Theoretical Physics, The Queen's University of Belfast, Belfast BT7 1NN, Northern Ireland, UK
Department of Applied Maths and Theoretical Physics, The Queen's University of Belfast, Belfast BT7 1NN, UK
School of Mathematics and Physics, The Queens University of Belfast, Belfast BT7 1NN, Northern Ireland, UK Queen's University
Department of Applied Mathematics and Theoretical Physics, The Queens University of Belfast, Belfast BT7 1NN, UK
Department of Applied Mathematics & Theoretical Physics, The Queen's University of Belfast, Belfast BT7 1NN, Northern Ireland
Department of Applied Mathematics and Theoretical Physics, Queen's University, Belfast, UK
Queen's University of Belfast, Belfast, N. Ireland, UK
A Comparison of Theoretical mg vi Emission Line Strengths with Active-Region Observations From Serts
A Comparison of Theoretical Si <Emphasis Type="SmallCaps">VIII</Emphasis> Emission Line Ratios with Observations from Serts
Auroral and nebular emission lines of [SII] in the optical spectra of planetary nebulae
Breit-Pauli R-matrix calculation of fine-structure effective collision strengths for the electron impact excitation of Mg V
Collision Strengths and Effective Collision Strengths for Transitions within the Ground-state Configuration of S III
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