|
|
|
|
|
|
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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
wWh7vtUW8y79YjxK
