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On the Absence of Core Luminosity–Core-Dominance Parameter (PC – R) Correlation in Radio Galaxies and BL Lacs

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dc.contributor.author Alhassan, J.A
dc.contributor.author Ubachukwu, A A
dc.contributor.author Odo, F C
dc.date.accessioned 2018-10-31T08:23:45Z
dc.date.available 2018-10-31T08:23:45Z
dc.date.issued 2013-01-28
dc.identifier.citation Alhassan, J.A , Ubachukwu, A A & Odo, F C (2013) On the Absence of Core Luminosity–Core-Dominance Parameter (PC – R) Correlation in Radio Galaxies and BL Lacs. J. Astrophys. Astr. 34, 61–67 en_US
dc.identifier.uri http://repository.unn.edu.ng/xmlui/handle/123456789/7534
dc.description.abstract We have presented an alternative interpretation for the absence of correlation in the relationship between the core radio power (PC) and core-dominance parameter (R) for a sample of BL Lacs and radio galaxies found in Fan & Zhang (Astron. Astrophys. 407, 89 (2003)). This is contrary to the predictions of the relativistic beaming and radio source orientation models in which the core luminosity is expected to be Doppler-boosted relative to the extended luminosity which is generally assumed to be isotropic. Our analysis of the PC − R data indicates a strong luminosity selection effect (reminiscent of bright source samples due to Malmquist bias) in the sample. In particular, we showed that a strong PC − R correlation exists above some redshift cut-off which may correspond to the flux limit of the sample used. en_US
dc.language.iso en en_US
dc.publisher Indian Academy of Sciences en_US
dc.subject Bl Lacertae Objects en_US
dc.subject General-Quasars—Galaxies en_US
dc.subject Seyfert—Galaxies en_US
dc.subject Jets en_US
dc.title On the Absence of Core Luminosity–Core-Dominance Parameter (PC – R) Correlation in Radio Galaxies and BL Lacs en_US
dc.type Article en_US


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