Zobrazeno 1 - 10
of 35
pro vyhledávání: '"K. T. S. Brazier"'
Autor:
K. T. S. Brazier, Simon Johnston
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 305:671-679
We collate the evidence for rotation-powered neutron stars that are visible as X-ray sources and not as radio pulsars. Quantitative upper limits exist for the radio fluxes of eight objects, revealing a population at least an order of magnitude less l
Autor:
K. T. S. Brazier, Werner Becker
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 284:335-340
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 281:1033-1037
Autor:
K. T. S. Brazier
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 268:709-712
Autor:
D. A. Kniffen, C. E. Fichtel, J. R. Mattox, H. A. Mayer-Hasselwander, Yiing Lin, J. M. Fierro, K. T. S. Brazier, P. L. Nolan, C. von Montigny, D. L. Bertsch, H. I. Nel, Peter F. Michelson, E. J. Schneid, Stanley D. Hunter, P. Sreekumar, Gottfried Kanbach, R. C. Hartman, D. J. Thompson
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 268:517-520
Autor:
S. M. Rayner, D J Orford, K. E. Turver, V. G. Mannings, A. Carraminana, P. J. Edwards, P. M. Chadwick, K. T. S. Brazier, S.M. Bradbury, K. J. Orford, C. C. G. Bowden, Nigel Dipper, E. W. Lincoln, T. J. L. McComb
Publikováno v:
Journal of Physics G: Nuclear and Particle Physics. 18:413-421
The authors' observations of Cygnus X-3 in 1981-88 have suggested that sporadic 12.6 ms pulsed very high energy gamma rays are produced at or near the maximum (phase 0.6) in the 4.8 h X-ray cycle. Cygnus X-3 was observed with the Durham University Ma
Autor:
Nigel Dipper, E. W. Lincoln, T. J. L. McComb, K. E. Turver, K. T. S. Brazier, P. M. Chadwick, A. Carraminana, K. J. Orford, S. M. Rayner, V. G. Mannings
Publikováno v:
Nuclear Physics B - Proceedings Supplements. 14:250-255
The design of two types of very high energy (VHE) gamma ray telescope which have the capability to enhance the gamma ray signal is discussed. The performance of the array of Cerenkov light telescopes operated at Dugway from 1981 – 1984 to provide w
Autor:
E. W. Lincoln, T. J. L. McComb, K. T. S. Brazier, Nigel Dipper, S. M. Rayner, K. E. Turver, A. Carraminana, V. G. Mannings, K. J. Orford, P. M. Chadwick
Publikováno v:
Nuclear Physics B - Proceedings Supplements. 14:196-199
We report observations of the X-ray pulsar 1E2259+586 made in 1988 October using the very high energy gamma ray telescope operating in La Palma. We find evidence significant at the 5.3 × 10 −5 level for the emission of 400 GeV gamma rays pulsating
Autor:
Gottfried Kanbach, K. T. S. Brazier, P. L. Nolan, D. J. Thompson, Olaf Reimer, A. Carraminana
The EGRET telescope has repeatedly observed 3EG J1835+5918 as a bright and steady source of high-energy gamma-ray radiation which has not yet been indentified. EGRET data from CGRO observation cycle 1 to 7 have been reanalysed above 100 MeV and above
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8b3fd153e5e588699fed392860fa3709
Publikováno v:
AIP Conference Proceedings.
The source 3EG J1835+5918 was discovered early in the CGRO mission by EGRET as a bright unidentified γ-ray source outside the galactic plane. Especially remarkable, it has not been possible to identify this object with any known counterpart in any o