... A massive eclipsing binary system Consists of a mass donor star and a compact object, surrounded by the precessing accretion ...

... white dwarfs (WDs), and this mass loss can induce instability in planetary systems as the planet:star mass ratio increases ...

... of the nebulae are intermediate-mass stars with mainsequence masses in the range M ... general, and the theory of the evolution of intermediate-mass stars, in particular ... The PN central-star masses taken from different sources can differ greatly. ...

... study of late evolutionary stages of intermediate-mass stars (of the order of 1-3 ... At this stage, stars intensely lose mass and, in about a hundred thousand years ... to the problem of late-type stars' variability, mass loss, maser emission, and ...

... most of the Giant Molecular Clouds and massive star forming regions in the northern ... structure of the protoplanetary disk surrounding three young intermediate mass stars ...

... we had evolved on a planet around a massive star, what `color' would our eye's see ... Massive stars use up their fuel much faster - in some cases less than 100 million ...

... in the characteristics of stars (their total luminosity, color, mass function, and ... the SFR accelerates, since the evolution of stars with masses exceeding 0.4M o (i.e ...

... The neutron-star masses presented in Fig. 1 are already given in [8], and we do not ... m LR/m. (8) The change of the star's mass m during a single stage in the model with ...

... ultraviolet radiation from a single massive star is sufficient to destroy all the H2 ... and subsequently grows by accreting the surrounding gas to become a massive star ...

... H.-Th. Janka et al. "Explosion Mechanisms of Massive Stars" astro-ph/0212314 . ... Daniel Schaerer "The massive star IMF" astro-ph/0208227 . ... A. Heger et al. "Massive Star Evolution Through the Ages" astro-ph/0211062 . ...