|
|
|
|
|
|
943 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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
qmArR1yyrAYFZVGp