Simultaneous X-Ray and TeV Observations of a Rapid Flare from Markarian 421

Mrk 421 was observed for about 2 days with BeppoSAX in 1998 April as part of a worldwide multiwavelength campaign. A large, well-defined flare was observed in X-rays. The same flare was observed simultaneously at TeV energies by the Whipple Observatory gamma-ray telescope. These data provide (1) the...

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Veröffentlicht in:The Astrophysical journal 1999-12, Vol.526 (2), p.L81-L84
Hauptverfasser: Maraschi, L, Fossati, G, Tavecchio, F, Chiappetti, L, Celotti, A, Ghisellini, G, Grandi, P, Pian, E, Tagliaferri, G, Treves, A, Breslin, A. C, Buckley, J. H, Carter-Lewis, D. A, Catanese, M, Cawley, M. F, Fegan, D. J, Fegan, S, Finley, J, Gaidos, J, Hall, T, Hillas, A. M, Krennrich, F, Lessard, R. W, Masterson, C, Moriarty, P, Quinn, J, Rose, J, Samuelson, F, Weekes, T. C, Urry, C. M, Takahashi, T
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Sprache:eng
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Zusammenfassung:Mrk 421 was observed for about 2 days with BeppoSAX in 1998 April as part of a worldwide multiwavelength campaign. A large, well-defined flare was observed in X-rays. The same flare was observed simultaneously at TeV energies by the Whipple Observatory gamma-ray telescope. These data provide (1) the first evidence that the X-ray and TeV intensities are well correlated on timescales of hours and (2) the first exactly simultaneous X-ray and TeV spectra. The results imply that the X-ray and TeV photons derive from the same region and from the same population of relativistic electrons. The physical parameters deduced from a homogeneous synchrotron self-Compton model for the spectral energy distribution yield electron cooling times close to the observed variability timescales.
ISSN:1538-4357
0004-637X
1538-4357
DOI:10.1086/312370