Context. Cygnus X-3 (Cyg X-3) is a well-known microquasar producing variable emission at all wavelengths. Cyg X-3 is a prominent X-ray binary producing relativistic jets, and studying its high energy emission is crucial for the understanding of the fundamental acceleration processes in accreting compact objects. Aims. Our goal is to study extreme particle acceleration and gamma-ray production above 100 MeV during special spectral states of Cyg X-3 usually characterized by a low hard X-ray flux and enhanced soft X-ray states. Methods. We observed Cyg X-3 with the AGILE satellite in extended time intervals from 2009 Jun.-Jul., and 2009 Nov.-2010 Jul. We report here the results of the AGILE gamma-ray monitoring of Cyg X-3 as well as the results from extensive multiwavelength campaigns involving radio (RATAN-600, AMI-LA and Metsahovi Radio Observatories) and X-ray monitoring data (XTE and Swift). Results. We detect a series of repeated gamma-ray flaring activity from Cyg X-3 that correlate with the soft X-ray states and episodes of decreasing or non-detectable hard X-ray emission. Furthermore, we detect gamma-ray enhanced emission that tends to be associated with radio flares greater than 1 Jy at 15 GHz, confirming a trend already detected in previous observations. The source remained active above 100 MeV for an extended period of time (almost 1.5 months in 2009 Jun.-Jul. and 1 month in 2010 May). We study in detail the short timescale gamma-ray flares that occurred before or near the radio peaks. Conclusions. Our results confirm the transient nature of the extreme particle acceleration from the microquasar Cyg X-3. A series of repeated gamma-ray flares shows correlations with radio and X-ray emission confirming a well established trend of emission. We compare our results with Fermi-LAT and MAGIC TeV observations of Cyg X-3.
AGILE detection of Cygnus X-3 gamma-ray active states during the period mid-2009/mid-2010 / Bulgarelli A; Tavani M; Chen AW; Evangelista Y; Trifoglio M; Gianotti F; Piano G; Sabatini S; Striani E; Pooley G; Trushkin S; Nizhelskij NA; McCollough M; Koljonen KII; Hannikainen D; Lahteenmaki A; Tammi J; Lavonen N; Steeghs D; Aboudan A; Argan A; Barbiellini G; Campana R; Caraveo P; Cattaneo PW; Cocco V; Contessi T; Costa E; DAmmando F; Del Monte E; De Paris G; Di Cocco G; Donnarumma I; Feroci M; Fiorini M; Fuschino F; Galli M; Giuliani A; Giusti M; Labanti C; Lapshov I; Lazzarotto F; Lipari P; Longo F; Marisaldi M; Mereghetti S; Morelli E; Moretti E; Morselli A; Pacciani L; Pellizzoni A; Perotti F; Picozza P; Pilia M; Prest M; Pucella G; Rapisarda M; Rappoldi A; Rubini A; Soffitta P; Trois A; Vallazza E; Vercellone S; Vittorini V; Zambra A; Zanello D; Giommi P; Pittori C; Verrecchia F; Santolamazza P; Lucarelli F; Colafrancesco S; Salotti L. - In: ASTRONOMY & ASTROPHYSICS. - ISSN 1432-0746. - STAMPA. - 538:(2012), pp. A63.1-A63.14. [10.1051/0004-6361/201016129]
AGILE detection of Cygnus X-3 gamma-ray active states during the period mid-2009/mid-2010
D'AMMANDO, FILIPPO;
2012
Abstract
Context. Cygnus X-3 (Cyg X-3) is a well-known microquasar producing variable emission at all wavelengths. Cyg X-3 is a prominent X-ray binary producing relativistic jets, and studying its high energy emission is crucial for the understanding of the fundamental acceleration processes in accreting compact objects. Aims. Our goal is to study extreme particle acceleration and gamma-ray production above 100 MeV during special spectral states of Cyg X-3 usually characterized by a low hard X-ray flux and enhanced soft X-ray states. Methods. We observed Cyg X-3 with the AGILE satellite in extended time intervals from 2009 Jun.-Jul., and 2009 Nov.-2010 Jul. We report here the results of the AGILE gamma-ray monitoring of Cyg X-3 as well as the results from extensive multiwavelength campaigns involving radio (RATAN-600, AMI-LA and Metsahovi Radio Observatories) and X-ray monitoring data (XTE and Swift). Results. We detect a series of repeated gamma-ray flaring activity from Cyg X-3 that correlate with the soft X-ray states and episodes of decreasing or non-detectable hard X-ray emission. Furthermore, we detect gamma-ray enhanced emission that tends to be associated with radio flares greater than 1 Jy at 15 GHz, confirming a trend already detected in previous observations. The source remained active above 100 MeV for an extended period of time (almost 1.5 months in 2009 Jun.-Jul. and 1 month in 2010 May). We study in detail the short timescale gamma-ray flares that occurred before or near the radio peaks. Conclusions. Our results confirm the transient nature of the extreme particle acceleration from the microquasar Cyg X-3. A series of repeated gamma-ray flares shows correlations with radio and X-ray emission confirming a well established trend of emission. We compare our results with Fermi-LAT and MAGIC TeV observations of Cyg X-3.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
