|
|
|
|
|
|
1073 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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
bE0HrmzyhKRT4ym5
