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Supernova remnants: on new ways to understand the cosmic ray physics | Oleh Petruk, INAF-Osservatorio Astronomico di Palermo 15:30
Supernova remnants: on new ways to understand the cosmic ray physics | Oleh Petruk, INAF-Osservatorio Astronomico di Palermo
Mar 2@15:30–16:30
I will talk about two new possibilities to analyse the observational data on non-thermal emission of cosmic rays accelerated in supernova remnants (SNRs). The first one is related to the polarization images of SNRs. In fact, the polarized radio emission has been mapped with great detail in several Galactic supernova remnants, but has not yet been exploited to the extent
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Flaring star-disk magnetic channels in Orion star-forming region | Fabio Reale, Universita’ di Palermo 16:00
Flaring star-disk magnetic channels in Orion star-forming region | Fabio Reale, Universita’ di Palermo
Mar 8@16:00–17:00
It is debated whether the long and intense flares observed on the PMS stars in Orion involve single and very long magnetic channels or much flatter loop arcades. This question is important because the long flaring channels may be so long as to connect the star to the circumstellar disk. In this work a new method solves the question ….
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Ripetizione tesi Tutone 15:30
Ripetizione tesi Tutone
Mar 15@15:30–17:00
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