|
|
|
|
|
|
1092 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
|
eNq9mFFv2jAQx9/5FFHeScgKajoFqo21G1KrMlq0aS+VSQ4wM3Z6toHu088hdIMpUVdT94GHxMn54vv7d3+cnG+WzFsBSip414+Clu8BT0VG+azrj+8um7F/3mskC7Iie4+dBq0gOvO9lBEpu34xGkyAcBl8v776BOZ9QL/X8BIxWUCqDp7TirLgC5Hza5IXz3jJStDMW4Kai6zr51pt73qJVGiy6K0F/pQ5SSEJd3f2Rxf37f37SVgE+4+oWgJeET6rDDpFq5ipRgSu+kTBTOBjZej0vhPFdilTOQIpNKYwJGo+RLGiGWTVH0CYBKtJpuvsFnDFQBWTVAYP06W0ik0WZDOCh0F1zh/MaF9tVLPVjE7juBXFcXwaxZHVVLi3UtV1WMowvT9pn5x12uEUQ4ETqsxbzWz705smKEGZuVga6dIVSMuaDQUqwhxVi8r+oeYczYPw8KwqMipzRh6Dhcxtl4ogMcOAhgzuPqT4gjs0rGJmzf6JzzVj4QuzHu9I4ijjAlR9obmqAcrlyHYh+oIr2NRX1I6BarPTIj3cMseF/SV4Nf+HesJoaos6QyMNUo1Hg1rSvQ0lPhIJY3SHiW+UZ2ItXx8/++V2lH2+JWhN9++033Ws99UPo6qabnShUeQQGiRReQxpBnwqjmWMEWp1qD8ydS/RrV8SKWFQ45ialiAy2nwyeM7U725nlQOVQT9f3NkK56sGfLzdXlaGpln3qeR2kHZBfqPS2rxfrvly07uy0hqreTJXKpfvw5BB1IGFcZCBZrOApObPzdv1gr2+7M7kO2n+pRkqqeoo9UnZKF9cPdut+JxDONb17t7fuevKORRqOKIcJbWdsXVw8fq4/mt5naU9POCLu2m29pQoKrgrd6QnNXQ8okGYsvJLNIi4mU5pzclLrSyTsDz16TWSsDjx6TV+A4aRDOM=
pNtGaAwBDqAvvQy9
