Zobrazeno 1 - 7
of 7
pro vyhledávání: '"V. J. Mantle"'
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
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
Autor:
V. J. Mantle, G. T. Bath
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 202:151-157
Publikováno v:
Cataclysmic Variables and Related Objects ISBN: 9789400971202
It is now well established, following the classic work of Smak, Warner and Nather, that discs in dwarf novae possess an anisotropic radiation pattern responsible for the hump, or shoulder, that occurs. prior to eclipse in the quiescent state, and, in
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d48d35b413525e8b25a1ed4736550ed8
https://doi.org/10.1007/978-94-009-7118-9_10
https://doi.org/10.1007/978-94-009-7118-9_10
Autor:
V. J. Mantle
Publikováno v:
Cataclysmic Variables and Low-Mass X-Ray Binaries ISBN: 9789401088497
It is now well established that the eruptions characteristic of dwarf novae result from changes in the luminosity of the accretion disc centred around the white dwarf component of these systems. These luminosity variations are most successfully accou
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::4deaaa743c55713008141bbd3cf74f60
https://doi.org/10.1007/978-94-009-5319-2_35
https://doi.org/10.1007/978-94-009-5319-2_35
Publikováno v:
Cataclysmic Variables and Related Objects ISBN: 9789400971202
Following earlier work of Lynden-Bell & Pringle (1974) and Lightman (1974a, 1974b), Bath & Pringle (1981) have presented a simple method for studying the time-dependent evolution of viscous accretion discs. These models are axisymmetric, with the ver
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::3cf27cd3e6d8e69403baae39f2147c21
https://doi.org/10.1007/978-94-009-7118-9_9
https://doi.org/10.1007/978-94-009-7118-9_9