Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2438
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dc.contributor.authorGhosh, K. K-
dc.contributor.authorSoundararajaperumal, S-
dc.date.accessioned2008-06-17T05:13:07Z-
dc.date.available2008-06-17T05:13:07Z-
dc.date.issued1992-11-
dc.identifier.citationA&A, Vol. 265, pp. 413 - 416en
dc.identifier.urihttp://hdl.handle.net/2248/2438-
dc.description.abstractFor 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-raysen
dc.format.extent506738 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherEDP Sciencesen
dc.relation.urihttp://adsabs.harvard.edu/abs/1992A%26A...265..413Gen
dc.subjectLUMINOSITYen
dc.subjectQUASARS, X RAY SPECTRAen
dc.subjectASTRONOMICAL MODELSen
dc.subjectEXOSAT SATELLITEen
dc.subjectSPECTRUM ANALYSISen
dc.titleFirst X-ray spectrum of the most luminous quasar PKS 2126 - 158en
dc.typeArticleen
Appears in Collections:IIAP Publications

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