Issue |
A&A
Volume 383, Number 1, FebruaryIII 2002
|
|
---|---|---|
Page(s) | L5 - L8 | |
Section | Letters | |
DOI | https://doi.org/10.1051/0004-6361:20011811 | |
Published online | 15 February 2002 |
Letter to the Editor
A superburst from GX 3+1
SRON National Institute for Space Research, Sorbonnelaan 2, 3584 CA Utrecht, The Netherlands Astronomical Institute, Utrecht University, PO Box 80000, 3508 TA Utrecht, The Netherlands
Corresponding author: erikk@sron.nl
Received:
23
November
2001
Accepted:
18
December
2001
I found one long X-ray flare from the X-ray burster GX 3+1 in almost 6 years of
observations with the RXTE All Sky Monitor (ASM).
The event had a peak flux of about 1.1 Crab (1.5–12 keV), lasted between
4.4 and 16.2 hours and exhibited a fluence
of more than about 51041 erg for a source distance of 5 kpc. During the
exponential-like decay, with an exponential decay time of 1.6 hours, spectral softening is seen.
The total ASM effective exposure time on GX 3+1 is estimated to be around a year.
The flare bears all the characteristics of the recently discovered so-called superbursts in other
X-ray burst sources.
Key words: accretion, accretion disks / binaries: close / stars: individual (GX 3+1) / stars: neutron / X-rays: bursts
© ESO, 2002
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