Binaire X
Une binaire X est formée d'une étoile « normale » orbitant autour d'une étoile à neutrons ou d'un trou noir avec une courte période. Le rayonnement X provient de l'énorme quantité d'énergie dégagée par l'accrétion de la matière de l'étoile autour de l'objet compact.
Uses material from the Wikipedia article "Binaire X", which is released under the Creative Commons BY-SA 3.0.| Objet céleste | Distance | Wiki | ||
|---|---|---|---|---|
| CXOU J061705.3+222127 | Binaire X | 5000 | ||
| GHJ2008 3 | Low Mass X-ray Binary | K | 26000 | |
| Gliese 3095 | Binaire X | 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 | [x] |
| 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 | [x] |
| V821 Arae | Low Mass X-ray Binary, High Mass X-ray Binary | 27000 | [x] | |
| X Persei | High Mass X-ray Binary | O | 1394 | |
| XTE J1748-288 | Low Mass X-ray Binary | 26000 | ||
| XTE J1752-223 | Binaire X, Low Mass X-ray Binary | 17000 | ||
| XTE J1755-324 | Low Mass X-ray Binary | 15000 | ||
| XTE J1817-330 | Binaire X, 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 |