X線連星
X線連星 (X-ray binary) はX線星ともいわれ、中性子星やブラックホールを伴星にもつ近接連星のことで、特にX線を強く放射することが知られている。X線は100万度以上の高温状態あるいはシンクロトロン放射などで生成される。
Uses material from the Wikipedia article "X線連星", which is released under the Creative Commons BY-SA 3.0.| 天体 | 距離 | ウィキ | ||
|---|---|---|---|---|
| CXOU J061705.3+222127 | X線連星 | 5000 | ||
| GHJ2008 3 | Low Mass X-ray Binary | K | 26000 | |
| Gliese 3095 | X線連星 | 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 | |
| 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 | |
| XTE J1748-288 | Low Mass X-ray Binary | 26000 | ||
| XTE J1752-223 | X線連星, Low Mass X-ray Binary | 17000 | ||
| XTE J1755-324 | Low Mass X-ray Binary | 15000 | ||
| XTE J1817-330 | X線連星, 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 |