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- 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
- Appears in Collections:
- 7. KISTI 연구성과 > 학술지 발표논문
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