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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Bibliographic Details
Main Authors:	Shabani, Fayezeh (Author) , Grebel, Eva K. (Author) , Pasquali, Anna (Author) , Gouliermis, Dimitrios A. (Author)
Format:	Article (Journal)
Language:	English
Published:	2018 May 16
In:	Monthly notices of the Royal Astronomical Society Year: 2018, Volume: 478, Issue: 3, Pages: 3590-3604
ISSN:	1365-2966
DOI:	10.1093/mnras/sty1277
Online Access:	Verlag, Volltext: http://dx.doi.org/10.1093/mnras/sty1277 Verlag, Volltext: https://academic.oup.com/mnras/article/478/3/3590/4996800
Author Notes:	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

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Summary:	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
Item Description:	Gesehen am 05.02.2019
Physical Description:	Online Resource
ISSN:	1365-2966
DOI:	10.1093/mnras/sty1277