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

Overview of SRG/eROSITA results in the Eastern Galactic hemisphere

8 Jul 2024, 15:00
40m
Europaurum (Aurum)

Europaurum

Aurum

Largo Gardone Riviera, Pescara, Italy
Invited talk in a parallel session High energy astrophysics High energy astrophysics

Speaker

Marat Gilfanov (MPA, Garching & IKI, Moscow)

Description

After more than two years of scanning the sky the eROSITA X-ray telescope aboard SRG orbital observatory produced the best ever X-ray maps of the sky and discovered more than three million X-ray sources, of which about 20% are stars with active coronas in the Milky Way, and most of the rest are galaxies with active nuclei, quasars and clusters of galaxies. eROSITA detected over 10^3 sources that changed their luminosity by more than an order of magnitude, including about a hundred tidal disruption events. Two tidal disruption events are associated with IceCube neutrinos. SRG/eROSITA samples of quasars and galaxy clusters will make it possible to study the large-scale structure of the Universe at z~1 and measure its cosmological parameters. I will review some of the SRG/eROSITA results in the Eastern Galactic hemisphere.

Primary author

Marat Gilfanov (MPA, Garching & IKI, Moscow)

Presentation materials

There are no materials yet.