|
|
|
|
|
|
1077 vues
Simulation des orbitres de deux étoiles massives O dans Cyg OB2#9 et des observations de XMM- Newton et Swift de l'émission des rayons X par ce système binaire. © NASA/ GSFC
|
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
CBWVKPxz6FE3SLs6
