2006A&A...445..313G

Query : 2006A&A...445..313G

2006A&A...445..313G - Astronomy and Astrophysics, volume 445, 313-321 (2006/1-1)

Two years of INTEGRAL monitoring of the soft gamma-ray repeater SGR 1806-20: from quiescence to frenzy.

GOETZ D., MEREGHETTI S., MOLKOV S., HURLEY K., MIRABEL I.F., SUNYAEV R., WEIDENSPOINTNER G., BRANDT S., DEL SANTO M., FEROCI M., GOEGUES E., VON KIENLIN A., VAN DER KLIS M., KOUVELIOTOU C., LUND N., PIZZICHINI G., UBERTINI P., WINKLER C. and WOODS P.M.

Abstract (from CDS):

SGR 1806-20 has been observed for more than 2 years with the INTEGRAL satellite. In this period the source went from a quiescent state into a very active one culminating in a giant flare on December 27, 2004. Here we report on the properties of all the short bursts detected with INTEGRAL before the giant flare. We derive their number-intensity distribution and confirm the hardness-intensity correlation for the bursts found by Goetz et al. (2004A&A...417L..45G). Our sample includes a very bright outburst that occurred on October 5, 2004, during which over one hundred bursts were emitted in 10 minutes, involving an energy release of 3x10⁴²erg. We present a detailed analysis of it and discuss our results in the framework of the magnetar model.

Abstract Copyright: ∼

Journal keyword(s): gamma rays: bursts - gamma rays: observations - stars: pulsars: general - stars: pulsars: individual: SGR 1806-20

Simbad objects: 3

Full paper

View the references in ADS

Number of rows : 3

N	Identifier	Otype	ICRS (J2000) RA	ICRS (J2000) DEC	Sp type	#ref 1850 - 2023	#notes
1	PSR B0525-66	Psr	05 26 00.7	-66 04 35	~	534	1
2	PSR J1808-2024	Psr	18 08 39.32	-20 24 40.1	~	1200	2
3	GBS 1900+14	gB	19 07 13	+09 19.6	~	832	0

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