|
|
|
|
|
|
1058 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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
StKYPn5egGPDLLew