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The 0.1–100 keV spectrum and variability of Mrk 421 in a high state.

Authors :
Malizia, A.
Capalbi, M.
Fiore, F.
Giommi, P.
Gandolfi, G.
Tesseri, A.
Antonelli, L.A.
Butler, R.C.
Celidonio, G.
Coletta, A.
Di Ciolo, L.
Muller, J.M.
Piro, L.
Rebecchi, S.
Ricci, D.
Ricci, R.
Smith, M.
Torroni, V.
Source :
Monthly Notices of the Royal Astronomical Society; 2/11/2000, Vol. 312 Issue 1, p123-129, 7p, 1 Chart, 9 Graphs
Publication Year :
2000

Abstract

The results of a BeppoSAX target of opportunity (TOO) observation of the BL Lac object Mrk 421 during a high-intensity state are reported and compared with monitoring X-ray data collected with the BeppoSAX Wide Field Cameras (WFC) and the RXTE All Sky Monitor (ASM). The 0.1–100 keV spectrum of Mrk 421 shows continuous convex curvature that can be interpreted as the high-energy end of the synchrotron emission. The source shows significant short-term temporal and spectral variability, which can be interpreted in terms of synchrotron cooling. The comparison of our results with those of previous observations when the source was a factor 3–5 fainter shows evidence for strong spectral variability, with the maximum of the synchrotron power shifting to higher energy during high states. This behaviour suggests an increase in the number of energetic electrons during high states. [ABSTRACT FROM AUTHOR]

Details

Language :
English
ISSN :
00358711
Volume :
312
Issue :
1
Database :
Complementary Index
Journal :
Monthly Notices of the Royal Astronomical Society
Publication Type :
Academic Journal
Accession number :
5892124
Full Text :
https://doi.org/10.1046/j.1365-8711.2000.03106.x