Multifrequency Behaviour of Galactic and Extragalactic Novae
Rosa Poggiani
TL;DR
This paper reviews the multifrequency observational data of galactic and extragalactic novae, highlighting new phenomena such as GeV gamma-ray emissions and emphasizing the importance of multi-wavelength studies in understanding nova eruptions.
Contribution
It provides a comprehensive overview of the multifrequency behaviour of novae, integrating optical, radio, infrared, X-ray, and gamma-ray observations to reveal new phenomena.
Findings
Detection of GeV gamma-ray emission from novae
Multi-wavelength observations uncover new physical phenomena
Enhanced understanding of nova eruption mechanisms
Abstract
The outbursts of novae are among the strongest explosions in the Universe. The eruptions involve physical processes that span the whole electromagnetic spectrum, demanding multifrequency observations. The photometric and spectroscopic observations in the optical domain are combined with radio, infrared, X-ray and gamma ray observations, allowing to discover new phenomena, like the GeV gamma ray emission.
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