|
|
|
|
|
|
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
912 vues
|
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
nHfgk3JjzjbB53Xb
