Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
University of Central Lancashire, United Kingdom
University of Manchester, NRAL
University of Manchester Nuffield Radio Astronomy Laboratories, Jodrell Bank, Macclesfield, Cheshire SK11 9DL
Department of Physics, Astronomy and Mathematics, University of Central Lancashire, Preston PR1 2HE, UK.
Centre for Astrophysics, University of Central Lancashire, Preston, Lancashire, PR1 2HE, UK
Centre for Astrophysics, The University of Central Lancashire, Preston, PR1 2HE, UK
Department of Physics, Keele University, Keele, Staffordshire ST5 5BG
University of Manchester, NRAL, Jodrell Bank, Macclesfield, Cheshire SK11 9DL; Physics Department, Keele University, Keele, Staffordshire ST5 5BG
Astrophysics Research Institute, Liverpool John Moores University, Twelve Quays House, Birkenhead L41 1LD
Centre for Astrophysics, University of Central Lancashire, Preston PR1 2HE
Keele, University
Astrophysics Research Institute, Liverpool John Moores University, Twelve Quays House, Egerton Wharf, Birkenhead CH41 1LD
Department of Physics, Keele University, Keele, Staffordshire, ST5 5BG, UK ; Astrophysics Research Institute, Twelve Quays House, Egerton Wharf, Birkenhead, L41 1LD, UK of Physics, Keele University, Keele, Staffs, ST5 5BG, UK; Astrophysics Research Institute, Liverpool John Moores University, Twelve Quays House, Egerton Wharf, Birkenhead, CH41 1LD, UK
Astrophysics Research Institute, Liverpool John Moores University, Twelve Quays House, Egerton Wharf, Birkenhead, CH41 1LD; Astrophysics Group, Physics Department, School of Chemistry and Physics, Keele University, Keele, ST5 5BG
Centre for Astrophysics, University of Central Lancashire, Preston, PR1 2HE
Space Science & Technology Department, CCLRC Rutherford Appleton Laboratory, Chilton, Didcot, Oxfordshire OX11 0QX, UK
Observatoire de Paris, 5, pl. J. Janssen, 92195, Meudon, France
Physics Department, Keele University, Keele ST5 5BG
Universit
A 1.19 day UV Photometric Period in Nova LMC 2009?
A possible detection of diffuse extended X-ray emission in the environment of the globular cluster NGC 6779
A radio detection of V Sagittae
A Search for CO J = 2 → 1 Emission from the Metal Rich Globular Cluster NGC 6356
A Search for Radio Emission from Galactic Supersoft X-ray Sources
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