Zobrazeno 1 - 10
of 135
pro vyhledávání: '"G. T. Bath"'
Autor:
G. T. Bath
Publikováno v:
Radiation Hydrodynamics in Stars and Compact Objects ISBN: 9783540167648
At outburst the classical nova generates an extended optically-thick wind driven by radiation pressure in the continuum. At maximum light the optical luminosity is close to the Eddington-limit. The subsequent decline illustrates the interaction betwe
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::000621a4fdc1d26256cb27922f473d06
https://doi.org/10.1007/3-540-16764-1_15
https://doi.org/10.1007/3-540-16764-1_15
Autor:
Michael Friedjung, G. T. Bath, T. Lloyd Evans, B. J. M. Hassall, Patricia A. Whitelock, A. W. Harris, Michel Dennefeld, M. A. J. Snijders, D. C. B. Whittet, John W. Menzies, A. Cassatella, M. Bode
Publikováno v:
Physics of Classical Novae ISBN: 9783540535003
We present results for IUE, optical and IR observations of Nova Muscae 1983, from early outburst to January 1986 obtained by the European IUE Target of Opportunity Team. A detailed description of the data will appear elsewhere (Hassall et al., 1989),
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::001d688463964f4a841c00907ebe2990
https://doi.org/10.1007/3-540-53500-4_124
https://doi.org/10.1007/3-540-53500-4_124
Autor:
H.J. van der Woerd, Philip A. Charles, G. Sonneborn, J. van Paradijs, B. J. M. Hassall, Tim Naylor, G. T. Bath
Publikováno v:
Astrophysics and Space Science. 130:371-376
We present ultraviolet and X-ray observations of the eclipsing SU UMa dwarf nova OY Car early in the decline from a superoutburst. From the UV emission line spectrum and lack of X-ray eclipse, we deduce the presence of an extended coronal region.
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 215:149-157
On examine l'hypothese de Papaloizou et Pringle ou les superbosses dans les systemes novae naines de type SU UMa sont generees par une modulation periodique de l'ecoulement dynamique du transfert de masse dans une binaire excentrique
Autor:
G. T. Bath
Publikováno v:
Symposium - International Astronomical Union. 73:173-192
Recent work on the physical processes resulting from mass transfer between the red and blue components of dwarf nova binaries is reviewed. The optical behaviour of the blue component's accretion disc suggests that it may be the infall, accretion ener
Autor:
J. C. B. Papaloizou, G. T. Bath
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 172:339-357
Autor:
G. T. Bath, J. E. Pringle
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 199:267-280
Autor:
Klaus Reinsch, Jeremy Bailey, P. A. Charles, Tim Naylor, B. Warner, Graham Berriman, G. T. Bath, B. J. M. Hassall
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 229:183-202
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 205:171-185
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 221:269-278
Etude de la forme des courbes de lumiere lors d'eruptions produites par des evenements avec transfert de masse dans des novae naines