The evolution of galaxy shapes in CANDELS: from prolate to discy
Abstract. We model the projected b/a-log a distributions of CANDELS star-forming main-sequence galaxies, where a (b) is the half-light semimajor (semiminor) ax
Enregistré dans:
| Auteurs principaux: | , |
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| Format: | Article (Journal) |
| Langue: | anglais |
| Publié: |
[April 2019]
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| In: |
Monthly notices of the Royal Astronomical Society
Year: 2019, Volume: 484, Numéro: 4, Pages: 5170-5191 |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/stz339 |
| Accès en ligne: | Verlag, Volltext: https://doi.org/10.1093/mnras/stz339 Verlag, Volltext: https://academic.oup.com/mnras/article/484/4/5170/5307087 
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| Notes sur l'auteur: | Haowen Zhang, Joel R. Primack, S. M. Faber, David C. Koo, Avishai Dekel, Zhu Chen, Daniel Ceverino, Yu-Yen Chang, Jerome J. Fang, Yicheng Guo, Lin Lin, Arjen van der Wel |
| Résumé: | Abstract. We model the projected b/a-log a distributions of CANDELS star-forming main-sequence galaxies, where a (b) is the half-light semimajor (semiminor) ax |
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| Description: | Advance access publication 2019 February 5 Gesehen am 23.04.2019 |
| Description matérielle: | Online Resource |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/stz339 |