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A year-long AGILE observation of Cygnus X-1 in hard spectral state

Authors :
Del Monte, E.
Feroci, M.
Evangelista, Y.
Costa, E.
Donnarumma, I.
Lapshov, I.
Lazzarotto, F.
Pacciani, L.
Rapisarda, M.
Soffitta, P.
Argan, A.
Barbiellini, G.
Boffelli, F.
Bulgarelli, A.
Caraveo, P.
Cattaneo, P. W.
Chen, A.
D'Ammando, F.
Di Cocco, G.
Fuschino, F.
Galli, M.
Gianotti, F.
Giuliani, A.
Labanti, C.
Lipari, P.
Longo, F.
Marisaldi, M.
Mereghetti, S.
Moretti, E.
Morselli, A.
Pellizzoni, A.
Perotti, F.
Piano, G.
Picozza, P.
Pilia, M.
Prest, M.
Pucella, G.
Rappoldi, A.
Sabatini, S.
Striani, E.
Tavani, M.
Trifoglio, M.
Trois, A.
Vallazza, E.
Vercellone, S.
Vittorini, V.
Zambra, A.
Antonelli, L. A.
Cutini, S.
Pittori, C.
Preger, B.
Santolamazza, P.
Verrecchia, F.
Giommi, P.
Salotti, L.
Source :
Astronomy and Astrophysics; September 2010, Vol. 520 Issue: 1
Publication Year :
2010

Abstract

Context. Cygnus X-1 (Cyg X-1) is a high mass X-ray binary system, known to be a black hole candidate and one of the brightest sources in the X-ray sky, which shows both variability on all timescales and frequent flares. The source spends most of the time in a hard spectral state, dominated by a power-law emission, with occasional transitions to the soft and intermediate states, where a strong blackbody component emerges.

Details

Language :
English
ISSN :
00046361 and 14320746
Volume :
520
Issue :
1
Database :
Supplemental Index
Journal :
Astronomy and Astrophysics
Publication Type :
Periodical
Accession number :
ejs53145561
Full Text :
https://doi.org/10.1051/0004-6361/200913104