Radio Microlensing: Past, Present & Near Future
| dc.creator | Koopmans, L. V. E. | |
| dc.creator | de Bruyn, A. G. | |
| dc.creator | Fassnacht, C. D. | |
| dc.creator | Wambsganss, J. | |
| dc.creator | Blandford, R. D. | |
| dc.creator | collaboration, + CLASS | |
| dc.date | 2000-11-01 | |
| dc.date.accessioned | 2026-07-07T01:56:21Z | |
| dc.date.available | 2026-07-07T01:56:21Z | |
| dc.description | Strongly correlated non-intrinsic variability between 5 and 8.5 GHz has been observed in one of the lensed images of the gravitational lens B1600+434. These non-intrinsic (i.e. `external') variations are interpreted as `radio-microlensing' of relativistic micro-arsec-scale jet components in the source at a redshift of z=1.59 by massive compact objects in the halo of the edge-on disk lens galaxy at z=0.41. We shortly summarize these observations and discuss several new observational and theoretical programs to investigate this new phenomenon in more detail. | |
| dc.description | 2 pages, LateX, 1 PostScript figures included, to appear in the proceedings of IAU Symposium 201 `New Cosmological Data and the Values of the Fundamental Parameters' (A. Lasenby and A. Wilkinson, eds.) | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0011034 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0011034 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/1969 | |
| dc.subject | Astrophysics | |
| dc.title | Radio Microlensing: Past, Present & Near Future | |
| dc.type | text |