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Título: | Properties of green valley galaxies in relation to their selection criteria |
Autor: | Nyiransengiyumva, Beatrice; Pović, Mirjana; Nkundabakura, Pheneas; Mahoro, Antoine | Palabras clave: | Galaxies: active Galaxies: star formation Galaxies: fundamental parameters Galaxies: evolution Ultraviolet: galaxies Methods: statistical |
Fecha de publicación: | 2021 | Editor: | Cambridge University Press | Citación: | Nuclear Activity in Galaxies Across Cosmic Time: 152-157 (2021) | Resumen: | The distribution of galaxies has been studied to show the difference between the blue cloud and red sequence and to define the green valley region. However, there are still many open questions regarding the importance of the green valley for understanding the morphological transformation and evolution of galaxies, how galaxies change from late-type to early-type and the role of AGN in galaxy formation and evolution scenario. The work focused on studying in more details the properties of green valley galaxies by testing the six most used selection criteria, differences between them, and how they may affect the main results and conclusions. The main findings are that, by selecting the green valley galaxies using different criteria, we are selecting different types of galaxies in terms of their stellar masses, sSFR, SFR, spectroscopic classification and morphological properties, where the difference was more significant for colour criteria than for sSFR and SFR vs. M* criteria. | Descripción: | Nuclear Activity in Galaxies Across Cosmic Time, Proceedings of the conference held 7-11 October 2019 in Addis Ababa, Ethiopia. Edited by Mirjana Pović et al. Proceedings of the International Astronomical Union, Volume 356, pp. 152-157 | Versión del editor: | http://dx.doi.org/10.1017/S1743921320002781 | URI: | http://hdl.handle.net/10261/252297 | DOI: | 10.1017/S1743921320002781 | Identificadores: | doi: 10.1017/S1743921320002781 isbn: 9781108492010 other SEV-2017-0709 |
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2021IAUS..356..152N.pdf | 435,41 kB | Adobe PDF | Visualizar/Abrir |
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