The Event Horizon Telescope collaboration has released the first high-energy gamma-ray outburst observed in over a decade from M87's powerful relativistic jet.
This Gamma-ray flare reveals a tremendous amount of energy in multiple wavelengths and helps constrain the size of the region responsible for the observed emission,
allowing researchers to study the physics surrounding M87's supermassive black hole.
The multi-wavelength campaign leveraged data from more than two dozen high-profile observational facilities, including Hubble Space Telescope and Chandra X-ray Observatory.
The flare lasted approximately three days and occupied a region roughly three light-days in size.
The discovery could create opportunities for future research and lead to breakthroughs in our understanding of the Universe,
The EHT collaboration comprises researchers from thirteen universities and institutes worldwide.
The study presents data from the second EHT observational campaign conducted in April 2018, which obtained nearly simultaneous spectra of the M87 galaxy with the broadest wavelength coverage ever collected.
The flare revealed that particles in supermassive black hole jets are accelerated in a unique way that cannot be explained by current theories.
This marks another important step towards understanding the universe.