|
|
|
|
|
|
1092 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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
AEvPMWf2SV0XQyf9