... We start with calculation of burst-like star formation in a galaxy assuming all stars to have been formed simultaneously. ... stars (presumably ``elliptical galaxies'' with no subsequent star formation) and a constant SFR of the second generation ...
... the energy the star would have at the circular orbit at a certain r and, hence, with a certain (recall that this corresponds to the minimum of the effective potential defined by ), expressed in units of the velocity component of the star in the direction ...
... Introduction . Observational Zoo of Binaries with Compact Stars . ... Principal Evolutionary States of Normal Stars . Main-sequence stars (stage I) . ... Main-sequence stars (stage I) . Post main sequence stars (stage II) . ...
... of the AF star, one of the most remarkable representatives of these stars, came up ... of the HeI/HI emission line stars in terms of young, massive stars is not the only ... star cluster (Eckart et al. 1993) is seemingly consistent with the other ...
... Up: Old neutron star distribution Previous: Old neutron star distribution ... neutron stars is computed for model galactic potential and initial neutron star ... stars are supposed to get their initial velocities during (asymmetric) supernova ...