Santiago Del Palacio
Santiago's research focuses in the study of astrophysical outflows associated with different sources, from massive stars to galaxies. He uses a combination of theoretical models and multi-frequency observations from radio wavelengths to very energetic gamma-rays. Santiago's main goal is to help to understand some of the most fascinating and extreme phenomena in the Universe, associated with relativistic particle acceleration and non-thermal emission processes.
Showing 10 publications
UPDATES ON THE GLITCHING PULSAR MONITORING CAMPAIGN PERFORMED FROM IAR
Evidence for non-thermal X-ray emission from the double Wolf-Rayet colliding-wind binary Apep
Probing the non-thermal physics of stellar bow shocks using radio observations
The radio detection and accretion properties of the peculiar nuclear transient AT 2019avd
A shared accretion instability for black holes and neutron stars
Search for particle acceleration in two massive Wolf-Rayet stars using uGMRT observations
The innermost jet in the hidden ultra-luminous X-ray source Cygnus X-3
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