We report the first detection with INTEGRAL of persistent hard X-ray emission (20 to 100 keV) from the Rapid Burster (MXB 1730-335), and describe its full spectrum from 3 to 100 keV. The source was detected on February/March 2003 during one of its recurrent outbursts. The source was clearly detected with a high signal to noise ratio during the single pointings and is well distinguished from the neighboring source GX 354-0. The 3-100 keV X-ray spectrum of the persistent emission is well described by a two-component model consisting of a blackbody plus a power-law with photon index ˜2.4. The estimated luminosity was ˜8.5 × 1036 erg s-1 in the 3-20 keV energy band and ˜1.3 × 1036 erg s-1 in the 20-100 keV energy range, for a distance of 8 kpc.
The discovery of hard X-ray emission in the persistent flux of the Rapid Burster
FARINELLI, Ruben;FRONTERA, Filippo;
2004
Abstract
We report the first detection with INTEGRAL of persistent hard X-ray emission (20 to 100 keV) from the Rapid Burster (MXB 1730-335), and describe its full spectrum from 3 to 100 keV. The source was detected on February/March 2003 during one of its recurrent outbursts. The source was clearly detected with a high signal to noise ratio during the single pointings and is well distinguished from the neighboring source GX 354-0. The 3-100 keV X-ray spectrum of the persistent emission is well described by a two-component model consisting of a blackbody plus a power-law with photon index ˜2.4. The estimated luminosity was ˜8.5 × 1036 erg s-1 in the 3-20 keV energy band and ˜1.3 × 1036 erg s-1 in the 20-100 keV energy range, for a distance of 8 kpc.I documenti in SFERA sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
