SciELO - Scientific Electronic Library Online

 
vol.55 issue2Interstellar absorption towards the Novae V339 Del and V5668 SGREnhanced mass loss rates in red supergiants and their impact on the circumstellar medium author indexsubject indexsearch form
Home Pagealphabetic serial listing  

Services on Demand

Journal

Article

Indicators

Related links

  • Have no similar articlesSimilars in SciELO

Share


Revista mexicana de astronomía y astrofísica

Print version ISSN 0185-1101

Abstract

ALHASSAN, Jibrin A.; UBACHUKWU, Augustine A.; ODO, Finbar C.  and  ONUCHUKWU, Chika C.. Relativistic beaming effects and structural asymmetries in highly asymmetric double radio sources. Rev. mex. astron. astrofis [online]. 2019, vol.55, n.2, pp.151-159.  Epub Nov 25, 2020. ISSN 0185-1101.  https://doi.org/10.22201/ia.01851101p.2019.55.02.03.

We have studied the comparative importance of the relativistic beaming model (RBM) and the density variation model (DVM) in our understanding of asymmetries in double radio sources, using their lobe separation ratio (Q) and flux density ratio (F ). Our result shows an F − Q correlation in the sense expected for the RBM but contrary to the DVM. We attributed the result for the DVM to varying beam power, as its efficiency is density profile-dependent. From the core-dominant parameter-linear size R − D relation for the RBM subsample, we found that sources in this subsample are beamed within an optimum cone angle ϕc ≈ 8◦. We posit that relativistic beaming is largely accountable for the observed structural asymmetries in radio sources, though other effects cannot be ruled out.

        · abstract in Spanish     · text in English