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BEGIN:VEVENT
DTSTART;TZID=Atlantic/Canary:20211102T113000
DTEND;TZID=Atlantic/Canary:20211102T123000
UID:iactalks-1513
X-WR-CALNAME: IAC Talks: Open Astronomy Seminars
X-ORIGINAL-URL: /iactalks/Talks/view/1513
CREATED:2021-11-02T11:30:00+00:00
X-WR-CALDESC: IAC Talks upcomming talks
SUMMARY:The high-energy view of Galactic particle accelerators
DESCRIPTION:The high-energy view of Galactic particle accelerators\nDr. Fab
 io Acero\n\nIn the aftermath of the cataclysmic explosion of massive stars
 , a vast zoology of source type is observed such as Supernova Remnants (SN
 Rs), pulsar wind nebulae, pulsars and ‘zombie’ pulsars. Due to
  high velocity shock-waves combined with a high magnetic field or fast rot
 ation in the case of pulsars, an efficient particle acceleration is achiev
 ed in those objects which are believed to be significant contributors to t
 he pool of Galactic cosmic rays.This seminar will start with a short intro
 duction on particle acceleration and SNR physics, present the current scie
 ntific questions, and what we’ve learned from high-energy observatio
 ns in the recent years.On a more technical note, I will also present a new
  analysis method to fully exploit the multi-dimensional (X, Y, Energy) nat
 ure of X-ray data. This blind source separation method draws from the most
  advanced signal processing techniques to capture and disentangle the weal
 th of information contained in deep archival observations.\n \nZoom:&
 nbsp;https://rediris.zoom.us/j/86212537380?pwd=MGdYSE1rVDAyVlVESFE5RWEwOVl
 qZz09Meeting ID: 862 1253 7380Passcode: 431670\n \nYouTube: http
 s://youtu.be/YwuCrGmp9_w
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