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Гравитационное микролинзирование

 а,  б
а Государственный научный центр Российской Федерации «Институт теоретической и экспериментальной физики им. А.И. Алиханова», ул. Б. Черемушкинская 25, Москва, 117259, Российская Федерация
б Московский Государственный университет им. М.В. Ломоносова, Государственный астрономический институт им. П.К.Штернберга, Университетский просп. 13, Москва, 119889, Российская Федерация

Изложены основы стандартной теории микролинзирования звезд, находящихся в нашей Галактике или в соседних галактиках, гравитационными линзами, расположенными между земным наблюдателем и этими звездами. В отличие от обзора Гуревича и др. [48] нами рассматривается главным образом микролинзирование на компактных объектах. Обсуждаются критерии отождествления событий микролинзирования, а также события, не удовлетворяющие этим критериям (несимметричные кривые блеска, эффект ахроматичности, эффекты поляризации). Подробно описаны результаты наблюдений микролинзирования группой МАСНО Большого Магелланова Облака (БМО) и Галактического балджа. Изложены результаты наблюдений БМО группой EROS и наблюдений Галактического балджа группой OGLE. Подробно обсуждается сопоставление результатов наблюдений с теорией.

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English fulltext is available at DOI: 10.1070/PU1998v041n10ABEH000460
PACS: 95.35.+d, 98.35.−a (все)
DOI: 10.3367/UFNr.0168.199810a.1041
URL: https://ufn.ru/ru/articles/1998/10/a/
000076871800001
Цитата: Захаров А Ф, Сажин М В "Гравитационное микролинзирование" УФН 168 1041–1082 (1998)
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English citation: Zakharov A F, Sazhin M V “Gravitational microlensingPhys. Usp. 41 945–982 (1998); DOI: 10.1070/PU1998v041n10ABEH000460

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