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- W2807271566 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." @default.
- W2807271566 created "2018-06-13" @default.
- W2807271566 creator A5063745055 @default.
- W2807271566 date "2018-01-30" @default.
- W2807271566 modified "2023-09-23" @default.
- W2807271566 title "On the multi-frequency emission and evolution of the white dwarf pulsar binary system AR Scorpii" @default.
- W2807271566 doi "https://doi.org/10.22323/1.306.0044" @default.
- W2807271566 hasPublicationYear "2018" @default.
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