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Context. Among intermediate-mass and massive stars, Be stars are the fastest rotators in the main sequence (MS) and, as such… Expand Two symmetrically coupled populations of N oscillators with inertia m display chaotic solutions with broken symmetry similar to… Expand We present a new radio survey of about 100 late-M and L dwarfs undertaken with the Very Large Array. The sample was chosen to… Expand INTRODUCTION: Rupture of the pectoralis major muscle appears to be increasing in athletes. However, the optimal treatment… Expand Recently, it was shown, that the mechanical model of a massive spinning particle proposed by Kuzenko, Lyakhovich and Segal in… Expand Abstract.We analyze the collective motion of suspensions of active rotators at low Reynolds numbers which interact… Expand Magnetic field amplification in astrophysics ultimately requires an understanding of MHD turbulence. Kinetic helicity has long… Expand We show that a steady mean-field dynamo in astrophysical rotators leads to an outflow of relative magnetic helicity and thus… Expand An experiment was conducted in an attempt to determine empirically how effective a number of expert clinicians were at… Expand Abstract. To determine the degree of damage induced by different modes of agitation during storage of platelets for 5 days in… Expand