Volume 306 -
XII Multifrequency Behaviour of High Energy Cosmic Sources Workshop (MULTIF2017) -
Astrophysics of High Energy Cosmic Sources
On the multi-frequency emission and evolution of the white dwarf pulsar binary system AR Scorpii
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Pre-published on:
January 30, 2018
Published on:
May 30, 2018
Abstract
The peculiar close binary system AR Scorpii, since its discovery in 2016, sparked huge interest due to its peculiar multi-frequency emission from radio frequencies to X-ray energies. The multi-frequency Spectral Energy Distribution (SED) from this system is dominated entirely by non-thermal emission from radio to X-ray energies, which resulted in several theoretical papers appearing in literature that attempted to explain the peculiar multi-frequency properties of this enigmatic source. In this paper, an emphatic theoretical framework will be presented to explain the multi-frequency SED of AR Sco, as well as a model to explain the possible origin and evolution of this enigmatic source.
DOI: https://doi.org/10.22323/1.306.0044
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Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.
Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.