AE Aquarii emission processes from radio to infrared

Bibcode
2005ASPC..330..341A
Abada-Simon, M.; Casares, J.; Evans, A.; Eyres, R.; Fender, R.; Garrington, S.; de Jager, O. C.; Kuno, N.; Martínez-País, I. G.; de Martino, D.; Matsuo, H.; Mouchet, M.; Pooley, G.; Ramsay, G.; Salama, A.; Schulz, B.
Bibliographical reference

The Astrophysics of Cataclysmic Variables and Related Objects, Proceedings of ASP Conference Vol. 330. Edited by J.-M. Hameury and J.-P. Lasota. San Francisco: Astronomical Society of the Pacific, 2005., p.341

Advertised on:
8
2005
Number of authors
16
IAC number of authors
0
Citations
1
Refereed citations
0
Description
AE Aquarii is a Magnetic Cataclysmic Variable (MCV) flaring at all wavelengths. The origin of its emission from radio to ≤ 10 μm is thought to be magneto-bremsstrahlung from both thermal and non-thermal electron energy distributions.
Type
Non-refereed

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