First broad band study of the mysterious source 1E 1743.1–2843
Context.In the last years, the persistent source 1E 1743.1–2843 has been observed in the X-rays, but never above 20 keV. In previous works, it was stressed that a possible high energy emission could give further indications on the accreting object nature which remains still unknown. Aims.We present...
Saved in:
Published in | Astronomy and astrophysics (Berlin) Vol. 456; no. 3; pp. 1105 - 1108 |
---|---|
Main Authors | , , , , , , |
Format | Journal Article |
Language | English |
Published |
Les Ulis
EDP Sciences
01.09.2006
|
Subjects | |
Online Access | Get full text |
Cover
Loading…
Summary: | Context.In the last years, the persistent source 1E 1743.1–2843 has been observed in the X-rays, but never above 20 keV. In previous works, it was stressed that a possible high energy emission could give further indications on the accreting object nature which remains still unknown. Aims.We present here more than two years of 1E 1743.1–2843 monitoring with INTEGRAL/IBIS as well as public XMM-Newton and Chandra X-ray observations. Methods.The temporal study in the 20–40 keV band shows a rather constant flux on few months time scale. Based on this result we have performed the broad-band spectral analysis using EPIC/IBIS non simultaneous data and ACIS-I/IBIS data collected during 2004. Results.In ~2 Ms, we report a detection of 6σ in the energy range 35–70 keV. The first broad-band study (2–70 keV) shows a steep slope (~3) and a black body temperature of 1.7 keV. Conclusions.Combining spectral parameters and discussion about the luminosity evaluations for different possible distances, our conclusions are in favour of a LMXB system with a neutron star at distance higher than the Galactic Centre, even though a firm conclusion can not be stated. |
---|---|
Bibliography: | istex:F0C8F2E39487DFCB87571E333621F927A7BF8751 ark:/67375/80W-QZ36R9VM-L other:2006A%26A...456.1105D publisher-ID:aa5029-06 ObjectType-Article-1 SourceType-Scholarly Journals-1 ObjectType-Feature-2 content type line 23 |
ISSN: | 0004-6361 1432-0746 |
DOI: | 10.1051/0004-6361:20065029 |