MAGIC search for VHEγ-ray emission from AE Aquarii in a multiwavelength context

J. Aleksić,S. Ansoldi,L. A. Antonelli,P. Antoranz,Ana Babić,P. Bangale,J. A. Barrio,J. Becerra González,W. Bednarek,E. Bernardini,B. Biasuzzi,A. Biland,O. Blanch,S. Bonnefoy,G. Bonnoli,F. Borracci,T. Bretz,E. Carmona,A. Carosi,P. Colin,E. Colombo,J. L. Contreras,J. Cortina,S. Covino,P. Da Vela,F. Dazzi,A. De Angelis,G. De Caneva,B. De Lotto,E. de Oña Wilhelmi,C. Delgado Mendez,M. Doert,D. Dominis Prester,D. Dorner,M. Doro,S. Einecke,D. Eisenacher,D. Elsäesser,M. V. Fonseca,L. Font,K. Frantzen,C. Fruck,D. Galindo, R. J. García López,M. Garczarczyk,D. Garrido Terrats,M. Gaug,N. Godinović,A. González Muñoz,S. R. Gozzini,D. Hadasch,Y. Hanabata,M. Hayashida,Javier Herrera,D. Hildebrand,J. Hose,Dario Hrupec,W. Idec,V. Kadenius,H. Kellermann,K. Kodani,Y. Konno,J. Krause,H. Kubo,J. Kushida,A. La Barbera,D. Lelas,N. Lewandowska, E. Lindfors,S. Lombardi,M. López,R. López-Coto,A. López-Oramas,E. Lorenz,Irene Albarrán Lozano,M. Makariev,K. Mallot,G. Maneva,N. Mankuzhiyil,K. Mannheim,L. Maraschi,B. Marcote,M. Mariotti,M. Martı́nez,D. Mazin,U. Menzel,J. M. Miranda,R. Mirzoyan,A. Moralejo,P. Munar-Adrover,D. Nakajima,A. Niedźwiecki,K. Nilsson,K. Nishijima,K. Noda,N. Nowak,R. Orito,A. Overkemping,S. Paiano, M. Palatiello, D. Paneque,R. Paoletti,J. M. Paredes,X. Paredes-Fortuny,M. Peršić,P. G. Prada Moroni,E. Prandini,S. Preziuso,I. Puljak,R. Reinthal,W. Rhode, M. Ribó,J. Rico,J. Rodriguez Garcia,S. Rügamer,A. Saggion,T. Saito,Koji Saito,K. Satalecka,V. Scalzotto,V. Scapin,C. Schultz,T. Schweizer,A. Sillanpää,J. Sitarek,Iva Šnidarić,D. Sobczyńska,F. Spanier,V. Stamatescu,A. Stamerra,T. Steinbring,J. Storz,M. Strzys,L. O. Takalo,H. Takami,F. Tavecchio,P. Temnikov,T. Terzić,D. Tescaro,M. Teshima,J. Thaele,O. Tibolla,D. F. Torres,Takeshi Toyama,A. Treves,M. Uellenbeck,P. Vogler,R. M. Wagner,R. Zanin,M. Bogosavljević,Z. Ioannou, Christopher W. Mauche, E. V. Palaiologou,M. A. Pérez-Torres,T. Tuominen

Astronomy and Astrophysics（2014）

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Abstract

Context. It has been claimed that the nova-like cataclysmic variable AE Aquarii (AE Aqr) is a very-high-energy (VHE, E> 100 GeV) source both on observational and theoretical grounds.

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Key words

ae aquarii,emission

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