Abstract
We report on RXTE-PCA observations of SLX 1746-311 during a ∼100 day outburst in April 2003. We present the 3-20 keV PCA energy spectra of the source and study evolution of spectral parameters. The burst spectrum is soft with Tin ∼1.3 keV at the beginning of the outburst. There is a clear evidence of a hard power law component throughout the outburst. There is also an indication of a broad iron line. The source exhibits three state transitions with considerable change in the hardness ratio at low count rates. We discuss the possible scenario under which this unusual behaviour can be explained.
| Original language | English |
|---|---|
| Pages (from-to) | 2788-2790 |
| Number of pages | 3 |
| Journal | Advances in Space Research |
| Volume | 38 |
| Issue number | 12 |
| DOIs | |
| Publication status | Published - 2006 |
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All Science Journal Classification (ASJC) codes
- Aerospace Engineering
- Space and Planetary Science
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SLX 1746-311 in outburst. / Narendranath, K. C Shyama; Ramadevi, M. C.; Sudhakar, M.; Bhattacharya, D.; Sreekumar, P.; Seetha, S.
In: Advances in Space Research, Vol. 38, No. 12, 2006, p. 2788-2790.Research output: Contribution to journal › Article
TY - JOUR
T1 - SLX 1746-311 in outburst
AU - Narendranath, K. C Shyama
AU - Ramadevi, M. C.
AU - Sudhakar, M.
AU - Bhattacharya, D.
AU - Sreekumar, P.
AU - Seetha, S.
PY - 2006
Y1 - 2006
N2 - We report on RXTE-PCA observations of SLX 1746-311 during a ∼100 day outburst in April 2003. We present the 3-20 keV PCA energy spectra of the source and study evolution of spectral parameters. The burst spectrum is soft with Tin ∼1.3 keV at the beginning of the outburst. There is a clear evidence of a hard power law component throughout the outburst. There is also an indication of a broad iron line. The source exhibits three state transitions with considerable change in the hardness ratio at low count rates. We discuss the possible scenario under which this unusual behaviour can be explained.
AB - We report on RXTE-PCA observations of SLX 1746-311 during a ∼100 day outburst in April 2003. We present the 3-20 keV PCA energy spectra of the source and study evolution of spectral parameters. The burst spectrum is soft with Tin ∼1.3 keV at the beginning of the outburst. There is a clear evidence of a hard power law component throughout the outburst. There is also an indication of a broad iron line. The source exhibits three state transitions with considerable change in the hardness ratio at low count rates. We discuss the possible scenario under which this unusual behaviour can be explained.
UR - http://www.scopus.com/inward/record.url?scp=33751162362&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=33751162362&partnerID=8YFLogxK
U2 - 10.1016/j.asr.2005.12.023
DO - 10.1016/j.asr.2005.12.023
M3 - Article
AN - SCOPUS:33751162362
VL - 38
SP - 2788
EP - 2790
JO - Advances in Space Research
JF - Advances in Space Research
SN - 0273-1177
IS - 12
ER -