Authors:
Khruzina, TS
Cherepashchuk, AM
Bisikalo, DV
Boyarchuk, AA
Kuznetsov, OA
Citation: Ts. Khruzina et al., Interpretation of light curves of IP Peg in a model with shockless interaction between the gas stream and disk, ASTRON REP, 45(7), 2001, pp. 538-552
Citation: Ii. Antokhin et Am. Cherepashchuk, Interpretation of the light curve of the eclipsing binary V444 Cyg on the set of convexo-concave functions, ASTRON REP, 45(5), 2001, pp. 371-381
Citation: Ii. Antokhin et Am. Cherepashchuk, Velocity field of the stellar wind of the Wolf-Rayet star in the V 444 Cygbinary system: A parametric model, ASTRON REP, 45(4), 2001, pp. 269-280
Citation: Am. Cherepashchuk, Wolf-Rayet stars and relativistic objects: Distinctions between the mass distributions in close binary systems, ASTRON REP, 45(2), 2001, pp. 120-137
Citation: Mm. Katsova et Am. Cherepashchuk, The quiescent X-ray emission of X-ray novae and the coronal emission of late-type stars, ASTRON REP, 44(12), 2000, pp. 804-814
Citation: Mb. Bogdanov et Am. Cherepashchuk, Reconstruction of the brightness distribution across a stellar disk from gravitational lensing caustic passage observations, ASTRON REP, 44(11), 2000, pp. 745-753
Citation: Mb. Bogdanov et Am. Cherepashchuk, Disk brightness distribution of a red giant from observations of gravitational microlensing, ASTRON REP, 43(9), 1999, pp. 601-607
Citation: Ts. Khruzina et Am. Cherepashchuk, Gravitational microlensing of binary stars: Analysis of the OGLE-5 and OGLE-6 light curves, ASTRON REP, 43(12), 1999, pp. 808-818