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http://hdl.handle.net/2248/2438
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DC Field | Value | Language |
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dc.contributor.author | Ghosh, K. K | - |
dc.contributor.author | Soundararajaperumal, S | - |
dc.date.accessioned | 2008-06-17T05:13:07Z | - |
dc.date.available | 2008-06-17T05:13:07Z | - |
dc.date.issued | 1992-11 | - |
dc.identifier.citation | A&A, Vol. 265, pp. 413 - 416 | en |
dc.identifier.uri | http://hdl.handle.net/2248/2438 | - |
dc.description.abstract | For the first time the detailed results of the spectral analysis of the X-ray (0.1 - 10 keV) spectrum of the luminous radio-loud quasar PKS 2126 - 158 are presented. Power law and fixed absorption model fits well with the spectrum. The parameters of this model suggest that this quasar is a flat spectrum source. Derived soft (0.1 - 2 keV) and hard (2 - 10 keV) X-ray luminosities of this quasar are (0.7 +/- 0.1) 10 exp 48 erg/s and (2.3 +/- 0.3) 10 exp 48 erg/s, respectively. No soft excess and low energy absorption have been detected in this source. Thermal bremsstrahlung model also fits well with the spectrum of PKS 2126 - 158 and the derived rest-frame temperature is 6.4 + 40 or -4 keV. This is the most luminous quasar which has been detected in the hard X-rays | en |
dc.format.extent | 506738 bytes | - |
dc.format.mimetype | application/pdf | - |
dc.language.iso | en | en |
dc.publisher | EDP Sciences | en |
dc.relation.uri | http://adsabs.harvard.edu/abs/1992A%26A...265..413G | en |
dc.subject | LUMINOSITY | en |
dc.subject | QUASARS, X RAY SPECTRA | en |
dc.subject | ASTRONOMICAL MODELS | en |
dc.subject | EXOSAT SATELLITE | en |
dc.subject | SPECTRUM ANALYSIS | en |
dc.title | First X-ray spectrum of the most luminous quasar PKS 2126 - 158 | en |
dc.type | Article | en |
Appears in Collections: | IIAP Publications |
Files in This Item:
File | Description | Size | Format | |
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Ghosh.part | 494.86 kB | Adobe PDF | View/Open |
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