Zobrazeno 1 - 10
of 22
pro vyhledávání: '"Frank M. Bateson"'
Autor:
Christie, Grant
Publikováno v:
Journal of the British Astronomical Association. Oct2007, Vol. 117 Issue 5, p275-275. 2/3p. 1 Black and White Photograph.
Autor:
Frank M. Bateson
Publikováno v:
Flares and Flashes ISBN: 9783540600572
This report provides a summary of flares observed visually in the dwarf novae V442 Cen, OY Car, TU Men and Z Cha. The flares precede an outburst by an average of around ten days.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::1097e1ad805aba6d3850b26f5dc7f484
https://doi.org/10.1007/3-540-60057-4_297
https://doi.org/10.1007/3-540-60057-4_297
Autor:
Frank M. Bateson, Tim Naylor, Koji Mukai, R. Stubbings, Coel Hellier, Danie Overbeek, Jonathan Kemp, A. Jones
We present the 45-yr record of EX Hya's lightcurve and discuss the characteristics of its 15 observed outbursts. We then concentrate on the 1998 outburst, reporting the first outburst X-ray observations. We discover an X-ray beat-cycle modulation, in
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1f7c09011717b24d939b660d5ed16858
Autor:
Frank M. Bateson
Publikováno v:
International Astronomical Union Colloquium. 151:286-287
This report provides a summary of flares observed visually in the dwarf novae V442 Cen, OY Car, TU Men and Z Cha. The flares precede an outburst by an average of around ten days.
Autor:
Frank M. Bateson
Publikováno v:
International Astronomical Union Colloquium. 46:89-95
The mean cycles and types of maxima for a number of dwarf novae are tabulated. It is shown that supermaxima are not confined to dwarf novae of short mean cycles. The decline rates for some stars are examined to ascertain if the orbital period, accura
Autor:
Frank M. Bateson
Publikováno v:
Vistas in Astronomy. 31:301-306
Autor:
Frank M. Bateson, I. M. Coulson, Brian Warner, P. A. Charles, Graham Berriman, K. Reinsch, Patricia A. Whitelock, Jeremy Bailey, Tim Naylor, A. R. Hyland
Publikováno v:
International Astronomical Union Colloquium. 93:365-369
We present optical and IR observations of the dwarf nova OY Car during the May 1985 superoutburst. From them we find that the superhump has a temperature of ~8000K and an area of order half the size of the red dwarf or accretion disk. We also compare
Autor:
Frank M. Bateson
Publikováno v:
Vistas in Astronomy. 31:297-300
Autor:
Patricia A. Whitelock, Brian Warner, A. R. Hyland, Tim Naylor, Frank M. Bateson, Jeremy Bailey, I. M. Coulson, Graham Berriman, K. Reinsch, Philip A. Charles
Publikováno v:
Cataclysmic Variables. Recent Multi-Frequency Observations and Theoretical Developments ISBN: 9789401081917
We present optical and IR observations of the dwarf nova OY Car during the May 1985 superoutburst. From them we find that the superhump has a temperature of ~8000K and an area of order half the size of the red dwarf or accretion disk. We also compare
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::4829cdb16838ef4485ef14eda983ea1c
https://doi.org/10.1007/978-94-009-3801-4_53
https://doi.org/10.1007/978-94-009-3801-4_53
Autor:
Frank M. Bateson
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 184:567-568