Modeling Quasar Microlensing

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F15%3A10398057" target="_blank" >RIV/00216208:11320/15:10398057 - isvavai.cz</a>
Result on the web
<a href="https://www.mff.cuni.cz/veda/konference/wds/proc/proc-contents.php?year=2015" target="_blank" >https://www.mff.cuni.cz/veda/konference/wds/proc/proc-contents.php?year=2015</a>
DOI - Digital Object Identifier
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Result language
angličtina
Original language name
Modeling Quasar Microlensing
Original language description
Light from a distant quasar passing in the vicinity of a foreground galaxy may be deflected by its gravitational field. According to the Fermat principle multiple macro-images of the quasar can then be observed. In addition, the light can be affected by the gravitational field of individual stars moving in the lensing galaxy, creating multiple micro-images. We cannot resolve them because of their small angular separation, but we can observe an associated increase of the flux. We will discuss how to model this phenomenon and related observable effects.
Czech name
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Czech description
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Project
Result was created during the realization of more than one project. More information in the Projects tab.
Continuities
P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)

Publication year
2015
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Article name in the collection
WDS 2015 — Proceedings of Contributed Papers — Physics
ISBN
978-80-7378-311-2
ISSN
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e-ISSN
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Number of pages
6
Pages from-to
21-26
Publisher name
MATFYZPRESS
Place of publication
Prague, 2015
Event location
Praha
Event date
Jun 2, 2015
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
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