|
|
|
|
|
|
1035 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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
pjpfb2ypeaKk4aKZ