X射线联星
X射线聯星是一类发出明亮X射线辐射的聯星,聯星系统中有一颗为致密星,通常为中子星或黑洞。它们的典型光度在1036-1038尔格/秒之间,比太阳全波段的光度高3到5个数量级。X射线聯星在靠近银心和银盘的方向分布比较集中,在球状星团中也有分布。
Uses material from the Wikipedia article "X射线联星", which is released under the Creative Commons BY-SA 3.0.Astronomical object | 距离 | Wiki | ||
---|---|---|---|---|
CXOU J061705.3+222127 | X射线联星 | 5000 | [x] | |
GHJ2008 3 | Low Mass X-ray Binary | K | 26000 | |
Gliese 3095 | X射线联星 | G | 148 | |
Great Annihilator | Low Mass X-ray Binary, High Mass X-ray Binary | 23000 | ||
GRS 1730-312 | Low Mass X-ray Binary | 21000 | ||
GRS 1758-258 | Low Mass X-ray Binary, High Mass X-ray Binary | 16000 | ||
GU Muscae | Low Mass X-ray Binary | K | 16500 | |
KV Ursae Majoris | Low Mass X-ray Binary | K | 6000 | |
MM Velorum | Low Mass X-ray Binary | G | 13000 | |
NOR X-1 | Low Mass X-ray Binary | ... | ||
QZ Vulpeculae | Low Mass X-ray Binary | K | 8800 | |
V1033 Scorpii | Low Mass X-ray Binary, High Mass X-ray Binary | F | 8000 | |
V1357 Cygni | High Mass X-ray Binary | O | 7500 | [x] |
V1487 Aquilae | Low Mass X-ray Binary | K | 8100 | [x] |
V2107 Ophiuchii | Low Mass X-ray Binary | K | 27000 | |
V381 Normae | Low Mass X-ray Binary | K | 17000 | |
V406 Vulpeculae | Low Mass X-ray Binary | G | 30000 | |
V4641 Sagittarii | Low Mass X-ray Binary | B | 30000 | |
V821 Arae | Low Mass X-ray Binary, High Mass X-ray Binary | 27000 | ||
X Persei | High Mass X-ray Binary | O | 1394 | [x] |
XTE J1748-288 | Low Mass X-ray Binary | 26000 | ||
XTE J1752-223 | X射线联星, Low Mass X-ray Binary | 17000 | ||
XTE J1755-324 | Low Mass X-ray Binary | 15000 | ||
XTE J1817-330 | X射线联星, Low Mass X-ray Binary | 10000 | ||
XTE J1818-245 | Low Mass X-ray Binary | 20000 | ||
XTE J1856+053 | Low Mass X-ray Binary, High Mass X-ray Binary | 21000 | ||
XTE J2012+381 | Low Mass X-ray Binary | 12000 |