... Kholtygin A.F., Igoshev A.P., Fabrika S.N. Statistics of magnetic fluxes of massive stars and enigma of origin of neutron stars magnetic fields . ...
... stars are very rare: for each such a star with a mass of more than 50 solar masses ... stars, which is based on their intrinsic property: when such a star decreases in ...
... LBV stars are the most massive stars in the final stages of evolution before exploding in of supernovae. ... star's temperature, measured on the spectra obtained on the 6-m BTA telescope (Fig.2), is 16000 K. In the infrared spectral ...
... Physics of Magnetic Stars . Proceedings of the International Conference, Nizhnij Arkhyz 28-31 August 2006. ... 8 . Balega Yu.Yu., Romanyuk I.I. Speech at the opening ceremony of the conference "Physics of magnetic stars" . 9 . ...
... star, marking the transition from the Main Sequence toward Wolf-Rayet (WR) stars ... of two very luminous stars in the M33 galaxy - LBV V532 and late WN star FSZ35 ... star, estimate its parameters and compare them to the corresponding parameters of ...
... The presence of a strong radial gradient of the magnetic field, averaged over the entire visible hemisphere of the star produces serious difficulties in the theoretical description - the star can not be stable in such fields. ...
... Luminous blue variable (LBV) stars are the most massive stars with 40-120 solar ... stars with infrared circular nebulae, found in the Spitzer survey (24 microns), a ... The star P Cygni itself was one of the brightest stars in the sky 400 years ago. ...
... stars, their multiplicity, the observed chemical composition anomalies, the effect of slow rotation of a number of magnetic ... stars from the considered sample, we conclude that, contrary to the current views, the proportion of double and multiple ...
... International Conference "Physics and Evolution of Magnetic and Related Stars" . ... Gautier Mathys . The (very) slow rotation of magnetic Ap stars. 10:30 - 11:10 . ... Magnetic stars in young clusters and associations. 11:40 - 12:20 . ...