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HEPRO X will cover all traditional topics of the series while placing a special emphasis on recent multi-messenger discoveries that have opened new windows on relativistic outflows.

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Core Topics:

• Relativistic outflows and particle acceleration

• Cosmic rays, gamma rays, and neutrinos

• Compact objects, pulsars, and their winds

• Microquasars and Active Galactic Nuclei (AGN)

• Gamma-ray bursts (GRBs)

• Multi-messenger astrophysics

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The 2027 program will feature dedicated sessions on groundbreaking recent observations, including:

• TeV gamma-ray afterglows of gamma-ray bursts.

• Ultra-high energy gamma-ray halos and other astrophysical enviroments powerd by pulsars.

• Variable ultra-high-energy gamma-ray emission from the microquasar Cygnus X-3.

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The meeting will highlight outstanding new results from currently operating facilities across the entire electromagnetic spectrum, as well as observations using different astrophysical messengers. At the same time, it will emphasize the capabilities of upcoming facilities and explore how they could revolutionize our understanding of relativistic outflows.

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• Agenda of the Scientific Conference

• Invited speakers

• Important Dates​

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Information will be updated regularly. Follow us to stay tuned!

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