6–9 Sept 2022
Physics Department, University "La Sapienza", Roma, Italy
Europe/Rome timezone

Evidence of hadronic origin of the gamma-ray emission from the nova RS Oph by the MAGIC telescopes

8 Sept 2022, 17:12
18m
Aula Conversi (Physics Department, University "La Sapienza", Roma, Italy)

Aula Conversi

Physics Department, University "La Sapienza", Roma, Italy

Speaker

David Green (Max Planck Institut für Physik)

Description

RS Ophiuchi (RS Oph) is a symbiotic recurrent nova that shows eruptive events roughly every 15 years. On August 8th August 2021, RS Oph erupted with its latest outburst. This event was detected with a wide range of multi-wavelength (MWL) instruments from radio up to very-high-energy (VHE) gamma rays. The MAGIC telescopes followed up on optical and high-energy triggers and initiated an observation campaign from August 9th till September 1st. RS Oph is the first nova detected in the VHE gamma-ray energy range. Together with optical, high energy, and VHE emission detected by MAGIC, it is evident that RS Oph conclusively accelerates hadrons during its eruption. We report on the detection of VHE gamma rays at a significant level of 13.2σ during the first 4 days of RS Oph with the MAGIC telescope. More importantly, we will present the MWL modeling which reveals a hadronic origin of the gamma-ray emission in this 2021 eruption, and its further implications for Galactic cosmic-rays.

Primary author

David Green (Max Planck Institut für Physik)

Co-authors

Dr Alicia López-Oramas (Instituto de Astrofísica de Canarias and Dpto. de Astrofísica) Dr Francesco Leone (National Institute for Astrophysics, Rome) Dr Julian Sitarek (University of Lodz, Faculty of Physics and Applied Informatics, Department of Astrophysics) Dr Rubén López-Coto (IAA-CSIC, Granada) Dr Vandad Fallah Ramazani (2 Ruhr-Universität Bochum, Fakultät für Physik und Astronomie, Astronomisches Institut (AIRUB))

Presentation materials