|
|
|
|
|
|
1052 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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
5KDY1LsEeGwvKKqX
