... and usually it is not seen as a radiopulsar since its pulse radiation is absorbed in the stellar wind of the normal star ... By this time, the normal star leaves the main sequence and the stellar wind strongly increases. ...
... non-conservative evolution (e.g., evolutionary stages with a strong stellar wind or those where the loss of the binary angular momentum occurs due to gravitational radiation or magnetic stellar wind) are treated using the well known prescriptions (see e.g ...
... The star wind velocity is estimated as km s (Howarth, 1983[ 67 ]). ... 1981)[ 135 ] discussed a model in which the companion is a relatively young pulsar losing energy via a relativistic wind ...
... CE), loss of orbital angular momentum at the expense of gravitational wave љ emission and the magnetic stellar wind, љ etc ... c) . loss of the orbital momentum due to magnetic wind; љ . (d) . evaporation of normal stars by radiopulsars; . (e) . ...
... that a massive star can lose more than of its initial mass during the evolution with a strong stellar wind (de Jager 1980 ... mass of the ZAMS star as high as since a substantial mass loss due to a strong stellar wind occurs for the most massive stars ...
... years, the star is in the ejector state usually unobservable due to absorption in the stellar wind from the normal star ... By this time, the normal star leaves the main sequence and the stellar wind is intensified. ...
... that a combination of dipole radiation, and wind luminosity, coupled with estimated ages and present spin parameters, imply that the magnetic field for SGR 1900+14 is less than 6 x 10^13 G and that the efficiency for conversion of wind luminosity to x-ray ...
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Ссылки http://xray.sai.msu.ru/~polar/html/coll2007/ppt/b-kogan.pdf -- 1845.3 Кб -- 19.06.2007 Похожие документы
... Just a box of rain, wind and water, . Sun and shower, wind and rain, . In and out the window like a moth before a flame. ... Just a box of rain, wind and water, . Sun and shower, wind and rain, . In and out the window like a moth before a flame. ...
... Всплеск 27 декабря 2004 г. по данным прибора Конус на спутнике Wind. Из работы Е.П. Мазеца и др. astro-ph/0502541 . ... Расположение аппаратов Wind и Коронас в момент вспышки. Видно, как Коронас мог зафиксировать отраженный от Луны сигнал. ...
... Gamma3=7 37 s: (1) For windaccreting systems we have: p eq:wind = 10:4 L \Gamma1 37 ... they are disk or windaccreting systems, less probable values (wind accretion in Be ...
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Ссылки http://xray.sai.msu.ru/~polar/html/publications/mag_field/p.ps -- 391.7 Кб -- 20.08.1999 Похожие документы