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The image jets modeling of gravitationally lensed sources

Published online by Cambridge University Press:  24 February 2011

Tatiana Larchenkova
Affiliation:
ASC of P. N. Lebedev Physical Institute, Profsoyuznaya str. 84/32, Moscow 117997, Russia email: [email protected]
Alexander Lutovinov
Affiliation:
Space Research Institute, Profsoyuznaya str. 84/32, Moscow 117997, Russia
Natalya Lyskova
Affiliation:
Moscow Physical-Technical Institute, Institutskyi per., 9, Dolgoprudnyi 141700, Russia
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Abstract

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The jets image modelling of gravitationally lensed sources have been performed. Several basic models of the lens mass distribution were considered, in particular, a singular isothermal ellipsoid, an isothermal ellipsoid with the core, different multi-components models with the galactic disk, halo and bulge. The obtained jet images were compared as with each other as with results of observations. A significant dependence of the Hubble constant on the model parameters was revealed for B0218+357, when the circular structure was took into account.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2011

References

Keeton, C. R. & Kochanek, C. S., 1998, ApJ, 495, 157CrossRefGoogle Scholar
Kuzmin, G., 1956, Sov. Astron, 33, 27Google Scholar
Larchenkova, T., Lutovinov, A., & Lyskova, N. 2011, Astron. Letters, in pressGoogle Scholar
Nair, S., Narasimha, D., & Rao, A. P., 1993, ApJ, 407, 46CrossRefGoogle Scholar
Patnaik, A. et al. , 1993, MNRAS, 261, 435CrossRefGoogle Scholar