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 17 publications
Joint ALMA/X-ray monitoring of the radio-quiet type 1 active galactic nucleus IC 4329A
Investigating the Role of Pre-supernova Massive Stars in the Acceleration of Galactic Cosmic Rays
PULSAR OBSERVATIONS AT LOW LATITUDES AND LOW FREQUENCIES
Timing irregularities and glitches from the pulsar monitoring campaign at IAR
Unraveling the Hybrid Origins of the X-Ray Nonthermal Emission from IGR J17091-3624
Study of Wolf-Rayet Stars Using uGMRT
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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