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공공누리This item is licensed Korea Open Government License

dc.contributor.author
A.Shatskiy
dc.contributor.author
Hansen
dc.date.accessioned
2019-08-28T07:41:13Z
dc.date.available
2019-08-28T07:41:13Z
dc.date.issued
2012-02-10
dc.identifier.issn
0035-8711
dc.identifier.uri
https://repository.kisti.re.kr/handle/10580/14093
dc.identifier.uri
http://www.ndsl.kr/ndsl/search/detail/article/articleSearchResultDetail.do?cn=NART62329759
dc.description.abstract
Inthispaperweproposeanewmethodforreconstructingthesurfacedensityofmatterinflatdisksofspiralgalaxies.Thesurfacedensityisexpressedthroughobservationalrotationvelocitycurvesofvisiblematterinthedisksofspiralgalaxies.Thenewmethodisnotbasedonquadratureofspecialfunctions.Thefoundsolutionisusedforprocessingandanalysisofobservationaldatafromseveralspiralgalaxies.Thenewmethodcanbeusedtomoreaccuratelyestimatetheamountofdarkmatterinspiralgalaxies.
dc.language
eng
dc.relation.ispartofseries
MonthlyNoticesoftheRoyalAstronomicalSociety
dc.title
A new integral representation for reconstructing the density distribution of matter in the discs of spiral galaxies using the rotation velocity curve in it
dc.citation.number
4
dc.citation.startPage
3071
dc.citation.volume
420
dc.subject.keyword
Analyticalandnumericalmethods
dc.subject.keyword
Galaxydisc
dc.subject.keyword
Darkmatter
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7. KISTI 연구성과 > 학술지 발표논문
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