The prevalence of star formation as a function of Galactocentric radius.
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| Title: | The prevalence of star formation as a function of Galactocentric radius. |
|---|---|
| Authors: | Ragan, S. E.1, S.Ragan@leeds.ac.uk, Moore, T. J. T.2, Eden, D. J.2, Hoare, M. G.1, Elia, D.3, Molinari, S.3 |
| Source: | Monthly Notices of the Royal Astronomical Society; 11/1/2016, Vol. 462 Issue 3, p3123-3129, 7p |
| Database: | Applied Science & Technology Source |
| FullText | Text: Availability: 0 |
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| Header | DbId: aci DbLabel: Applied Science & Technology Source An: 118703945 AccessLevel: 2 PubType: Academic Journal PubTypeId: academicJournal PreciseRelevancyScore: 0 |
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| PLink | https://search.ebscohost.com/login.aspx?direct=true&site=eds-live&db=aci&AN=118703945 |
| RecordInfo | BibRecord: BibEntity: Identifiers: – Type: doi Value: 10.1093/mnras/stw1870 Languages: – Code: eng Text: English PhysicalDescription: Pagination: PageCount: 7 StartPage: 3123 Titles: – TitleFull: The prevalence of star formation as a function of Galactocentric radius. Type: main BibRelationships: HasContributorRelationships: – PersonEntity: Name: NameFull: Ragan, S. E. – PersonEntity: Name: NameFull: Moore, T. J. T. – PersonEntity: Name: NameFull: Eden, D. J. – PersonEntity: Name: NameFull: Hoare, M. G. – PersonEntity: Name: NameFull: Elia, D. – PersonEntity: Name: NameFull: Molinari, S. IsPartOfRelationships: – BibEntity: Dates: – D: 01 M: 11 Text: 11/1/2016 Type: published Y: 2016 Identifiers: – Type: issn-print Value: 00358711 Numbering: – Type: volume Value: 462 – Type: issue Value: 3 Titles: – TitleFull: Monthly Notices of the Royal Astronomical Society Type: main |
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