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- W1963154489 abstract "We analyse the radiation pressure instability of the standard, optically thisc disc and propose it as an explanation of the obseved variability of the superluminal microquasar GRS 1915+105. The quantitave agreement with the observed outburst amplitudes is obtained under the assumption that substantial part of the energy is carried away by the jet." @default.
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- W1963154489 date "2000-04-25" @default.
- W1963154489 modified "2023-09-27" @default.
- W1963154489 title "Variability Model for the Microquasar GRS 1915+105" @default.
- W1963154489 hasPublicationYear "2000" @default.
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