Документ взят из кэша поисковой машины. Адрес оригинального документа : http://xray.sai.msu.ru/~mystery/articles/review/node53.html
Дата изменения: Sat Feb 22 23:56:44 1997
Дата индексирования: Tue Oct 2 14:47:42 2012
Кодировка:

Поисковые слова: m 11
The Number of Ejectors in Binaries next up previous contents index
Next: Why do Radiopulsars not Up: Ejectors in Massive Binary Previous: The Evolutionary Status of

The Number of Ejectors in Binaries

 

It is convenient to start with a situation in which the NS enters a binary system with a normal star losing matter in the form of a stellar wind.  Numerical simulation of the evolution of NS shows (Lipunov and Prokhorov, 1987[115]) that the fraction of ejecting stars in massive systems with normal components may be as high as several tens of percent of the total number of binary systems (see Figure 27). Below we describe some sources with appropriate properties.



Mike E. Prokhorov
Sat Feb 22 18:38:13 MSK 1997