Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Queen's University, Belfast, Northern Ireland
Department of Applied Mathematics and Theoretical Physics, The Queen's University of Belfast, Belfast BT7 1NN
Belfast, Queen's University, Belfast, Northern Ireland
Belfast, Queen's University, Northern Ireland
Belfast Queen's University
Belfast, Queen's Univ., United Kingdom
Delhi Univ., Delhi, India
Department of Applied Mathematics and Theoretical Physics, Queen's University of Belfast, Belfast BT7 1NN
Department of Appl. Math. & Theor. Phys., Queen's Univ., Belfast, UK
Department of Appl. Math. & Theor. Phys., Queen's University of Belfast, UK
School of Mathematics and Physics, The Queen's University of Belfast, Belfast BT7 1NN
Department of Applied Mathematics and Theoretical Physics, Queen's University, Belfast BT7 1NN, UK
Belfast, Queens University, Northern Ireland
Dept. of Appl. Math. & Theoretical Phys., Queen's Univ. of Belfast, Belfast, UK
Department of Applied Mathematics and Theoretical Physics, Queen's University, Belfast BT7 INN, Northern Ireland
Applied Mathematics and Theoretical Physics Department, Queen's University Belfast, Belfast BT7 1NN, Northern Ireland, UK
Department of Applied Mathematics and Theoretical Physics, The Queen's University of Belfast, Belfast BT7 1NN, Northern Ireland
Department of Applied Mathematics and Theoretical Physics, Queen's University, Belfast BT7 1NN
School of Mathematics and Physics, Queen's University of Belfast, Belfast BT7 1NN, UK
Queen's University of Belfast, Belfast, N. Ireland, UK
SERC, Daresbury Laboratory, Warrington, England
Department of Mathematics, Queen's University of Belfast, Northern Ireland
Queen's University Belfast
School of Mathematics and Physics, Queen's University Belfast, Belfast BT7 1NN, UK
Department of Applied Mathematics and Theoretical Physics, Quee
3s23p-3s3p2 transitions in SIV
Accurate F values of astrophysical interest for neutral carbon
Accurate oscillator strengths of astrophysical interest for neutral oxygen
Accurate transition probabilities for spectral lines of N III
An extremely peculiar hot subdwarf with a ten-thousand-fold excess of zirconium, yttrium, and strontium
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