1991
DOI: 10.1086/169776
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Possible detection of TeV gamma rays from AM Herculis

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Cited by 18 publications
(14 citation statements)
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“…Possible TeV emission from some magnetic CVs was announced in the past (Bhat et al 1991;Bowden et al 1992;Meintjes et al 1992), but was never confirmed by subsequent deeper observations (Lang et al 1998;Sidro et al 2008;López-Coto et al 2013). Indeed, models describing production of γ-ray emission from magnetic CVs have been developed (e.g., Schlegel et al 1995, and references therein; Bednarek & Pabich 2011), but they can hardly be applied to the two cases in our sample as they do not appear to host a white dwarf with a strong magnetic field (see Appendix).…”
Section: Discussionmentioning
confidence: 98%
“…Possible TeV emission from some magnetic CVs was announced in the past (Bhat et al 1991;Bowden et al 1992;Meintjes et al 1992), but was never confirmed by subsequent deeper observations (Lang et al 1998;Sidro et al 2008;López-Coto et al 2013). Indeed, models describing production of γ-ray emission from magnetic CVs have been developed (e.g., Schlegel et al 1995, and references therein; Bednarek & Pabich 2011), but they can hardly be applied to the two cases in our sample as they do not appear to host a white dwarf with a strong magnetic field (see Appendix).…”
Section: Discussionmentioning
confidence: 98%
“…At the beginning of the nineties of the last century, acceleration of particles by the rotating magnetic field of the WD in intermediate polars in the propeller regime -AE Aqr --detected by ground-based Cherenkov telescopes in the TeV passband (e.g. Meintjes et al 1992), and TeV emission from the polar AM Her detected by ground-based Cherenkov telescopes (Bhat et al 1991) -measurements never confirmed -were the main reasons of renewed interest for CVs in the high energy astrophysicists community.…”
Section: Renewed Interest For Cataclysmic Variablesmentioning
confidence: 99%
“…3 was operated during 1984-89. Using this system they observed a few Xray binaries (Cyg X-3, Her X-1, 4U0115+63), pulsars (Geminga, PSR 0355+54) and cataclysmic variables (Am Her) and other sources [20,21,22]. More details of the historic account of the above activities are documented in literature [23,24].…”
Section: Early Historymentioning
confidence: 99%