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0212U002351,
0111U003978
,
Theoretic and observational studies of the weak lensing phenomenon
Minakov Anatoliy Alexeevich,
10-02-2012
Institute of Radio Astronomy of Sciences of Ukraine
For the first time, characteristics of radiation were estimated for the extended structure surrounding the accretion disc of the Q2237+0305 quasar, namely, the upper limit for the energy contribution of the structure in different regions of the optical spectral range. A chapter "Gravitational lensing as a key to solving the dark matter problem" is prepared for publication in the joint monograph on the Program "Cosmicrophysics", which contains the key results obtained during 2009-2011. Numerical simulation of the high amplification events are fulfilled for various source models in two cases: with the appreciable dark matter content near the line of sight and for the finite-size microlens. Solutions of the problem of lensing by a complex lens for an arbitrary location of a microlens along the source-macrolens-observer path. Isophots for macroimages are built and the amplification rate for the complex lens was calculated.
Александров А.О.
Бєрдіна Л.А.
Баннікова О.Ю.
Вакулік В.Г.
Дудінов В.М.
Жданов В.І.
Железняк О.П.
Захожай В.А.
Конічек В.В.
Конторович В.М.
Кочетов О.Є.
Мінаков А.О.
Пташник Л.Г.
Сергеєв О.В.
Смирнов Г.В.
Федорова О.В.
Цвєткова.В.С.
Шульга В.М.
Шульга Д.В.
2020-04-02
Updated: 2025-12-07
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