Gopal-Krishna, ; Subramanian, K. (1996) Testing the lensing hypothesis for compact double radio sources and other milli-lensing candidates Astronomy & Astrophysics, 315 . pp. 343-347. ISSN 0004-6361
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Official URL: http://cdsads.u-strasbg.fr/abs/1996A&A...315..343G
Abstract
Condensed objects of ≈ 106 M⊙ could manifest themselves via their lensing action on the radio cores of background quasars, thus giving rise to compact double sources, or more complex small-separation lenses, on the milli-arcsecond scale. Such compact bodies could be dense cores of small galaxies or remnants of pregalactic stars which have been postulated as a candidate for the dark matter in the universe. Search for examples of milli-arcsecond scale lensing, either due to such remnants or dwarf galaxies, forms a central objective of several new VLBI projects which has already revealed a good candidate. Here we point out that the milli-lensing of superluminal cores of quasars/blazars, when it occurs, can lead to substantial changes in the apparent orientation, flux ratio and velocities of the image components over periods as short as a year. This is essentially because the proper motion of the sub-components of such cores is comparable to the image splitting scales. Hence VLBI monitoring programmes can provide a fairly simple test of the milli-lensing hypothesis.
Item Type: | Article |
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Source: | Copyright of this article belongs to EDP Sciences. |
Keywords: | Gravitational Lensing; Dark Matter; Galaxies: Jets; Galaxies: Active; Quasars: General; Radio Continuum: Galaxies |
ID Code: | 76546 |
Deposited On: | 04 Jan 2012 06:16 |
Last Modified: | 18 May 2016 20:09 |
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