Документ взят из кэша поисковой машины. Адрес
оригинального документа
: http://xray.sai.msu.ru/~raguzova/BeXcat/node1.html
Дата изменения: Tue Nov 4 16:42:11 2008 Дата индексирования: Tue Oct 2 02:33:45 2012 Кодировка: |
Be/X-ray binaries form the largest subclass of High Mass X-ray Binaries (HMXBs). These objects attract interests of specialists in several branches of astrophysics: stellar astrophysics, accretion theory, close binary evolution, etc. In recent years because of new X-ray satellites data available on these sources has greatly increased (see a recent review and references in paper by Negueruela (2005)). In this paper (which is an extended and updated version of Popov & Raguzova (2004)) we present a compilative catalogue of these sources and provide brief comments on each source in the sample.