 Limitation of the TTV technique for the detection of non-transiting planets G. Boué, M. Oshagh, M. Montalto, N. C. Santos Orbital couples: “Pas de deux” in the Solar System and in the Milky Way Type: Oral comunication |
 |
 |
 |
 |
 |
 |
 |
|
Limitation of the TTV technique for the detection of non-transiting planets G. Boué, M. Oshagh, M. Montalto, N. C. Santos Orbital couples: “Pas de deux” in the Solar System and in the Milky Way Type: Oral comunication |
@astro.up.pt
We use cookies to ensure that you get the best experience on our website, by continuing on this website you agree to the storing of cookies on your device. Learn more about our Privacy Policy .