... MicroBOKZ star tracker exceeds both the Russian and foreign analo gues in dimensio ... The tracker has a mass o f 600 g, power consumpt ion of 1 W and provides for ... The star trackers MicroBOKZ and BOKZM60/1000 are shown in fig. 1. ...
... Conclusion . Experiment: EVRIS INVESTIGATIONS OF OSCILLATIONS IN STARS . ... and internal structure of stars, measuring photometric microvariabilities induced by ... precision photometric observations of several bright stars during the cruise of the ...
... the available range of mass accretion rates, black hole masses, and spins ... mass can be much higher than 2-3 Msun, usually assumed in the collapsar model, and ... merger of a WR star with an ultra-compact companion, neutron star or black hole ...
... Date of discovery . 1979 . Mass (kg) . 1.91e+16 . Mass (Earth = 1) . 3.1961e-09 . ... Mass (kg) . 1.91e+16 . Mass (Earth = 1) . 3.1961e-09 . Radius (km) . 12.5x10x7.5 . ... The brighter dot to the left is a star. (Credit: Calvin J. Hamilton) . ...
... Seminar council . " Neutrino emmission from neutron stars " . A. D. Kaminker . ... emission mechanisms in different layers of neutron stars (NSs) are presented ... J0822-43 and PSR 1055-52, hotter for their ages, as very slowly low-mass cooling NSs ...
... M.Gilfanov , A.Bogdan Low-mass X-ray binary populations in galaxy outskirts ... Gilfanov , D.Pooley Spatially resolved star formation image and the ultraluminous x ... A.Bogdan Dependence of the low-mass X-ray binary population on stellar age ...
... with the local stars visible on a clear night, orbits the center of our home galaxy, a spiral disk of 200 billion stars we call ... Like the Milky Way, M31 is a giant spiral-shaped disk of stars, with a bulbous central hub of older stars. ...