Authors:
Bisikalo, DV
Boyarchuk, AA
Kilpio, AA
Kuznetsov, OA
Citation: Dv. Bisikalo et al., A possible manifestation of spiral shock waves in the accretion disks of cataclysmic variables, ASTRON REP, 45(9), 2001, pp. 676-685
Citation: Sy. Mel'Nikov, The dependence of the characteristics of the brightness variability of Herbig Ae/Be stars on the orientation of their star-disk systems, ASTRON REP, 45(9), 2001, pp. 686-691
Citation: Dp. Savokhin et al., Models for highly flattened, rapidly rotating cool stars in a Newtonian approximation, ASTRON REP, 45(9), 2001, pp. 692-699
Citation: Av. Loktin et Gv. Beshenov, Luminosity calibration for OB stars from Hipparcos trigonometric parallaxes, ASTRON REP, 45(9), 2001, pp. 711-717
Citation: Ea. Bruevich et al., Levels of coronal and chromospheric activity in late-type stars and various types of dynamo waves, ASTRON REP, 45(9), 2001, pp. 718-728
Citation: Vn. Krivodubskii, The structure of the global solar magnetic field excited by the turbulent dynamo mechanism, ASTRON REP, 45(9), 2001, pp. 738-745
Citation: Vi. Makarov et al., The increase in the magnetic flux from the polar regions of the sun over the last 120 years, ASTRON REP, 45(9), 2001, pp. 746-750
Citation: Yl. Bukhmastova, Properties of quasar-galaxy associations and gravitational mesolensing by halo objects, ASTRON REP, 45(8), 2001, pp. 581-590
Authors:
Bisikalo, DV
Boyarchuk, AA
Kil'pio, AA
Kuznetsov, OA
Chechetkin, VM
Citation: Dv. Bisikalo et al., The structure of matter flows in semi-detached binaries after the termination of mass transfer, ASTRON REP, 45(8), 2001, pp. 611-619
Citation: Av. Mordvinov et La. Plyusnina, Coherent structures in the dynamics of the large-scale solar magnetic field, ASTRON REP, 45(8), 2001, pp. 652-658
Citation: Av. Pynzar et Vi. Shishov, A correlation between the distributions of pulsars and emission measures in the galaxy, ASTRON REP, 45(7), 2001, pp. 502-509
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