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• W3100375295 abstract "<i>Context. <i/>The blazar 1 ES 1218+30.4 has been previously detected by the VERITAS and MAGIC telescopes in the very high energies. The new detection of VERITAS from December 2008 to April 2009 proves that 1 ES 1218+30.4 is not static, but shows short-time variability.<i>Aims. <i/>We show that the time variability may be explained in the context of a self-consistent synchrotron-self Compton model, while the long time observation do not necessarily require a time-resolved treatment.<i>Methods. <i/>The kinetic equations for electrons and photons in a plasma blob are solved numerically including Fermi acceleration for electrons as well as synchrotron radiation and Compton scattering.<i>Results. <i/>The light curve observed by VERITAS can be reproduced in our model by assuming a changing level of electron injection compared to the constant state of 1 ES 1218+30.4. The multiwavelength behaviour during an outburst becomes comprehensible by the model.<i>Conclusions. <i/>The long time measurements of VERITAS are still explainable via a constant emission in the SSC context, but the short outbursts each require a time-resolved treatment." @default.
• W3100375295 created "2020-11-23" @default.
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• W3100375295 date "2010-06-01" @default.
• W3100375295 modified "2023-09-25" @default.
• W3100375295 title "Modelling the variability of 1ES1218+30.4" @default.
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• W3100375295 doi "https://doi.org/10.1051/0004-6361/201014299" @default.
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