C. W. Mauche, M. Abada-Simon, J. -F. Desmurs, M. J. Dulude, Z. Ioannou, J. D. Neill, A. Price, N. Sidro, W. F. Welsh, the Center for Backyard Astrophysics, the American Association of Variable Star Observers
Published 2011-11-04Version 1
We provide a summary of results, obtained from a multiwavelength (TeV gamma-ray, X-ray, UV, optical, and radio) campaign of observations of AE Aqr conducted in 2005 August 28-September 2, on the nature and correlation of the flux variations in the various wavebands, the white dwarf spin evolution, the properties of the X-ray emission region, and the very low upper limits on the TeV gamma-ray flux.
Comments: 8 pages, 6 figures, uses mem.cls v1.9, submitted for inclusion in the proceedings of the conference "The Golden Age of CVs and Related Objects," reference: Mauche, C. W., et al. 2012, in "The Golden Age of Cataclysmic Variables and Related Objects," F. Giovannelli & L. Sabau-Graziati (Eds.), Mem. SAIt. 83, N. 2, in press
MAGIC search for VHE $γ$-ray emission from AE Aquarii in a multiwavelength context
Magnetars: the physics behind observations
The 2005 - 2010 multiwavelength campaign of OJ287
![QR code for arXiv:1111.1190 [astro-ph.HE]](http://oss.arxitics.com/images/favicon.svg)