1. Электронный научный архив УрФУ
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Please use this identifier to cite or link to this item: http://elar.urfu.ru/handle/10995/92273
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dc.contributor.authorSeleznev, A. F.en
dc.date.accessioned2020-10-20T16:35:06Z-
dc.date.available2020-10-20T16:35:06Z-
dc.date.issued2016-
dc.identifier.citationSeleznev A. F. Kernel density estimation in the study of star clusters / A. F. Seleznev. — DOI 10.1515/astro-2017-0129 // Baltic Astronomy. — 2016. — Iss. 25. — P. 267-274.en
dc.identifier.issn1392-0049-
dc.identifier.otherhttps://doi.org/10.1515/astro-2017-0129pdf
dc.identifier.other2-3good_DOI
dc.identifier.other01bfe65c-3827-45fa-a36d-db5eaf611246pure_uuid
dc.identifier.otherhttp://www.scopus.com/inward/record.url?partnerID=8YFLogxK&scp=85017620104m
dc.identifier.urihttp://elar.urfu.ru/handle/10995/92273-
dc.description.abstractThe kernel estimator method is used to evaluate the surface and spatial star number density in star clusters. Both density maps and radial density profiles are plotted. These estimates are used to derive the cluster size, the number of cluster stars and the cluster mass, and to study the cluster structure. The kernel estimator is also used to plot the luminosity function, mass function, the velocity distribution, and Hess diagrams for star clusters. The advantages of the kernel estimator method and technical details of its use are illustrated by modern results for the open cluster NGC 4337. © 2016, Lithuanian Astronomical Union. All rights reserved.en
dc.description.sponsorshipMinistry of Education and Science of the Russian Federation, Minobrnauka: 3.1781.2014/K, 01201465056en
dc.description.sponsorshipGovernment Council on Grants, Russian Federationen
dc.description.sponsorshipThis work was partially supported by the Ministry of Education and Science of the Russian Federation (state contract No. 3.1781.2014/K, registration number 01201465056). The travel to the conference was supported by Act 211 of the Government of the Russian Federation, agreement No. 02.A03.21.0006.en
dc.format.mimetypeapplication/pdfen
dc.language.isoenen
dc.publisherLithuanian Astronomical Unionen
dc.rightsinfo:eu-repo/semantics/openAccessen
dc.sourceBaltic Astronomyen
dc.subjectGLOBULAR CLUSTERS: GENERALen
dc.subjectMETHODS: STATISTICALen
dc.subjectOPEN CLUSTERS AND ASSOCIATIONS: GENERALen
dc.titleKernel density estimation in the study of star clustersen
dc.typeConference Paperen
dc.typeinfo:eu-repo/semantics/conferenceObjecten
dc.typeinfo:eu-repo/semantics/publishedVersionen
dc.identifier.doi10.1515/astro-2017-0129-
dc.identifier.scopus85017620104-
local.affiliationAstronomical Observatory, Ural Federal University, Mira str. 19, Ekaterinburg, 620002, Russian Federation
local.contributor.employeeSeleznev, A.F., Astronomical Observatory, Ural Federal University, Mira str. 19, Ekaterinburg, 620002, Russian Federation
local.description.firstpage267-
local.description.lastpage274-
local.issue25-
dc.identifier.wos000390981900004-
local.identifier.pure1451375-
local.identifier.eid2-s2.0-85017620104-
local.identifier.wosWOS:000390981900004-
Appears in Collections:Научные публикации ученых УрФУ, проиндексированные в SCOPUS и WoS CC

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