The evolutionary evidence for Be/black hole binaries

被引:0
|
作者
Raguzova, NV [1 ]
Lipunov, VM
机构
[1] Moscow MV Lomonosov State Univ, Fac Phys, Moscow 117234, Russia
[2] Moscow MV Lomonosov State Univ, Sternberg Astron Inst, Moscow 119899, Russia
关键词
stars : binaries : close; black hole physics; stars; emission-line; Be; stars : evolution;
D O I
暂无
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Using Monte Carlo simulation of the modern scenario of the evolution of binary systems (the "Scenario Machine"), we calculate the number of binary black holes with Be stars and their expected observational properties. So far, only two possible candidates for Be/BH binaries have been proposed among the observable sources, the superluminal source GRS 1915+105 in the Galaxy and RX J0117.6-7330 in SMC. Using the "Scenario Machine" we obtained an evolutionary track that can lead to the formation of such systems. The modern evolutionary scenario predicts the existence of binary black holes on eccentric orbits around Be stars and such systems may be discovered in the near future.
引用
收藏
页码:505 / 510
页数:6
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