Оригинальный обзор "Астрофизика одиночных нейтронных звезд: радиотихие нейтронные звезды и магнитары" (см. также обновляемую версия в формате PostScript ) . Нейтронные звезды . ... Новорожденные нейтронные звезды . ... Статья о свойствах молодых...
... stars will be written using roman figures (I-IV), whereas those of compact stars ... star remaining after the mass transfer in cases B and C of binary evolution; may ...
... stars left behind stellar evolution are (in the case of the most massive stars) NSs ... star's spin period P (or spin frequency ), its magnetic field strength B (or ... stars are assumed to collapse into a BH once their mass before the collapse is ...
... The star leaves the main sequence and goes toward the red (super)giant region in the Hertzsprung-Russell diagram (as before, the star still does not fill its RL). ...
... like star formation burst, one gets a Green function for any arbitrary star ... star formation at a particular redshift resulting in a stellar system which we call ... star formation history in the Universe by the fractional part of the luminous ...
... Stars with collapses to form NS of 1.4 M; when a BH with a mass of is formed, where is either the mass of the pre-collapsing star (in the case of low stellar wind mass-loss scenario), or the initial mass of the star (in teh case of the high stellar wind ...
... We have assumed a constant in time star formation rate and the total number of stars in the Galaxy, , to be such that the total mass of the galaxy is ; assuming the Salpeter mass function , we get . ...
... For Be-stars (i.e. those stars at the stage ``I'' whose mass increased during the ... giant post-MS stars (stage ``II''), we assume and for massive star we take maximum ...
... A MS-star that accretes matter during the first mass transfer is considered to be a rapidly rotating Be-star that is distinguished by its different stellar wind rate (see below). ...
... Evolution of the coalescence rate of double neutron stars (NS) and neutron star - black hole (BH) binaries are computed for model galaxies with different star formation rates. ...