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15:00
“Measuring the post-shock temperatures of heavy ions in SN 1987A”, Marco Miceli (UNIPA)
“Measuring the post-shock temperatures of heavy ions in SN 1987A”, Marco Miceli (UNIPA)
Jan 15 @ 15:00 – 16:00
The interaction of the shock waves originated from supernova explosions with the circumstellar medium provides crucial information on the physics of shock heating. Astrophysical shocks at all scales, from those in the heliosphere up to the cosmological shock waves, are typically collisionless and electrons, protons, and ions are expected to be heated at different temperatures. Although optical observations of Balmer-dominated
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