|
|
|
|
|
|
1128 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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
hLbTkn83t8XLvWpc
