7–12 Jul 2024
Aurum, the ‘Gabriele d’Annunzio’ University and ICRANet
Europe/Rome timezone

Magnetar Giant Flares

11 Jul 2024, 17:00
30m
M6 (Palazzo Micara of the ‘Gabriele d’Annunzio’ University)

M6

Palazzo Micara of the ‘Gabriele d’Annunzio’ University

Viale Pindaro, 42, Pescara
Invited talk in a parallel session Galactic and extragalactic magnetars: recent observations and theoretical progress Galactic and extragalactic magnetars: recent observations and theoretical progress

Speaker

Eric Burns

Description

Magnetars were discovered as soft gamma-ray repeaters by gamma-ray burst monitors. Their most energetic events are giant flares, seen as a bright, short flash followed by an exponentially-decaying periodic tail. There have been 3 such events seen in the Milky Way and Large Magellanic Cloud in ~60 years of observing. When these events occur in nearby galaxies their tail emission is undetectable, and they appear as short gamma-ray bursts. We have now identified 6 extragalactic magnetar giant flares, allowing for the first population studies on rates and host galaxy types, providing key information in the quest to understand their progenitors. We will discuss recent results and on-going work.

Primary author

Presentation materials