Search for star cluster age gradients across spiral arms of three LEGUS disc galaxies
ABSTRACT. One of the main theories for explaining the formation of spiral arms in galaxies is the stationary density wave theory. This theory predicts the exis
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| Hauptverfasser: | , , , |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
2018 May 16
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| In: |
Monthly notices of the Royal Astronomical Society
Year: 2018, Jahrgang: 478, Heft: 3, Pages: 3590-3604 |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/sty1277 |
| Online-Zugang: | Verlag, Volltext: http://dx.doi.org/10.1093/mnras/sty1277 Verlag, Volltext: https://academic.oup.com/mnras/article/478/3/3590/4996800 
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| Verfasserangaben: | F. Shabani, E.K. Grebel, A. Pasquali, E. D’Onghia, J.S. Gallagher, A. Adamo, M. Messa, B.G. Elmegreen, C. Dobbs, D.A. Gouliermis, D. Calzetti, K. Grasha, D.M. Elmegreen, M. Cignoni, D.A. Dale, A. Aloisi, L.J. Smith, M. Tosi, D.A. Thilker, J.C. Lee, E. Sabbi, H. Kim and A. Pellerin |
| Zusammenfassung: | ABSTRACT. One of the main theories for explaining the formation of spiral arms in galaxies is the stationary density wave theory. This theory predicts the exis |
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| Beschreibung: | Gesehen am 05.02.2019 |
| Beschreibung: | Online Resource |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/sty1277 |