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15:30
Hot Jupiters (and beyond) – A report on what I did during AstroFit fellowship | I. Pillitteri ( INAF OAPA )
@ Aula OAPA
Hot Jupiters (and beyond) – A report on what I did during AstroFit fellowship | I. Pillitteri ( INAF OAPA )
@ Aula OAPA
Dec 16 @ 15:30 – 16:30
In this talk I want to report on my research activity during the past two years at INAF-OAPa, which has been focused on the study of systems with hot Jupiters. In particular, I will show how hot Jupiters can affect the activity of their host stars, in two examples: HD 189733 and WASP-18. I will briefly report on results from
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15:30
Star-Planet magnetic interactions – A. F. Lanza ( INAF OACT )
Star-Planet magnetic interactions – A. F. Lanza ( INAF OACT )
Dec 17 @ 15:30 – 16:30
I shall review some phenomena possibly related to the magnetic interaction between late-type stars and close-in massive planets and discuss models proposed for their interpretation. I shall consider the possible effects of hot Jupiters on stellar chromospheric emission and on stellar rotation. On the other hand, magnetic reconnection between stellar and planetary magnetic fields may enhance the evaporation of the
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15:30
Non-thermal emission processes in shock acceleration events: application to SNRs and bow shocks | V. Pereira ( Univ. Complutense, Madrid )
@ Aula OAPA
Non-thermal emission processes in shock acceleration events: application to SNRs and bow shocks | V. Pereira ( Univ. Complutense, Madrid )
@ Aula OAPA
Dec 19 @ 15:30 – 16:30
High energy photons produced in the acceleration regions of strong shocks, such as supernova remnants (SNR) or bow shocks formed by runaway stars, are suggested to have a non-thermal origin. However, the efficiency of these processes is still debated. Here we aim to develop a non-thermal model by appealing to a mixed leptonic-hadronic scenario to explain the observational data obtained
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