SIMBAD references

2003MNRAS.342..909M - Mon. Not. R. Astron. Soc., 342, 909-914 (2003/July-1)

Discovery of type I X-ray bursts from the low-mass X-ray binary 4U 1708-40.

MIGLIARI S., DI SALVO T., BELLONI T., VAN DER KLIS M., FENDER R.P., CAMPANA S., KOUVELIOTOU C., MENDEZ M. and LEWIN W.H.G.

Abstract (from CDS):

We report the discovery of type I X-ray bursts from the low-mass X-ray binary 4U 1708-40 during the 100-ks observation performed by BeppoSAX on 1999 August 15-16. Six X-ray bursts have been observed. The unabsorbed 2-10 keV fluxes of the bursts range from ∼3 to 9x10–10 erg/cm2/s. A correlation between peak flux and fluence of the bursts is found, in agreement with the behaviour observed in other similar sources. There is a trend of the burst flux to increase with the time interval from the previous burst. From the value of the persistent flux we infer a mass accretion rate {formmu2}, which may correspond to the mixed hydrogen/helium burning regime triggered by thermally unstable hydrogen. We have also analysed a BeppoSAX observation performed on 2001 August 22 and previous RXTE observations of 4U 1708-40, where no bursts have been observed; we find persistent fluxes of more than a factor of 7 higher than the persistent flux observed during the BeppoSAX observation showing X-ray bursts.

Abstract Copyright: 2003 RAS

Journal keyword(s): accretion, accretion discs - stars: individual: 4U 1708-40 - stars: neutron - X-rays: bursts - X-rays: general

Simbad objects: 6

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