Interpretation of the light curves of “quiescent” X-ray novae in a model with a noncollisional interaction between the flow and disk. The XTE J1118+480 system T. S. KhruzinaA. M. CherepashchukO. A. Kuznetsov OriginalPaper Pages: 79 - 88
The evolution of close binary systems with intermediate-mass black holes and ultra-luminous X-ray sources A. V. TutukovA. V. Fedorova OriginalPaper Pages: 89 - 101
Gravitational darkening coefficients of the stars in the semidetached binary V Puppis E. A. AntokhinaE. V. SeifinaA. M. Cherepashchuk OriginalPaper Pages: 102 - 108
Radial-velocity curves and theoretical spectral-line profiles of the components of low-mass close X-ray binary systems E. A. AntokhinaA. M. CherepashchukV. V. Shimanskii OriginalPaper Pages: 109 - 126
Limits on the flux of ultrahigh-energy neutrinos from radio astronomical observations A. R. BeresnyakR. D. DagkesamanskiiV. V. Oreshko OriginalPaper Pages: 127 - 133
Limits on the mass of dark matter in the Sun from a model for the modern Sun and its previous evolution N. S. KardashevA. V. TutukovA. V. Fedorova OriginalPaper Pages: 134 - 143
The nature of decimeter-wave microburst emission V. M. BogodL. V. Yasnov OriginalPaper Pages: 144 - 154
Large-scale activity in solar eruptive events of October–November 2003 observed from SOHO/EIT data I. M. ChertokV. V. Grechnev OriginalPaper Pages: 155 - 166
