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Uspekhi Fizicheskikh Nauk, 2007, Volume 177, Number 11, Pages 1179–1206
DOI: https://doi.org/10.3367/UFNr.0177.200711b.1179 (Mi ufn529) 		 
This article is cited in 45 scientific papers (total in 45 papers)

REVIEWS OF TOPICAL PROBLEMS

Population synthesis in astrophysics

S. B. Popov, M. E. Prokhorov

Sternberg Astronomical Institute, Lomonosov Moscow State University
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DOI: https://doi.org/10.3367/UFNr.0177.200711b.1179
Abstract: Population synthesis is а method for numerical simulation of the population of objects with а complex evolution. This method is widely used in astrophysics. We consider its main applications to studying astronomical objects. Examples of modeling evolution are given for populations of close binaries and isolated neutron stars. Тhе application of the method to studying active galactic nuclei and the integral spectral characteristics of galaxies is briefly discussed. An extensive bibliography on all the topics covered is provided.
Received: July 17, 2006
Revised: June 1, 2007
English version:
Physics–Uspekhi, 2007, Volume 50, Issue 11, Pages 1123–1146
DOI: https://doi.org/10.1070/PU2007v050n11ABEH006179
Bibliographic databases:
Document Type: Article
PACS: 97.10.-q, 97.60.Jd, 97.80.-d
Language: Russian
Citation: S. B. Popov, M. E. Prokhorov, “Population synthesis in astrophysics”, UFN, 177:11 (2007), 1179–1206; Phys. Usp., 50:11 (2007), 1123–1146
Citation in format AMSBIB
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    • This publication is cited in the following 45 articles:
    Citing articles in Google Scholar: Russian citations, English citations
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