Chemical abundance of the LINER galaxy UGC 4805 with SDSS-IV MaNGA

Chemical abundance determinations in Low-Ionization Nuclear Line Regions (LINERs) are especially complex and uncertain because the nature of the ionizing source of this kind of object is unknown. In this work, we study the oxygen abundance in relation to the hydrogen abundance (O/H) of the gas phase...

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Detalles Bibliográficos
Autores principales:	Krabbe, Angela, Oliveira, C. B., Zinchenko, Igor A., Hernandez Jimenez, J. A., Dors, Oli L., Hägele, Guillermo Federico, Cardaci, Mónica Viviana, Telles, N. R.
Formato:	Articulo Preprint
Lenguaje:	Inglés
Publicado:	2021
Materias:	Ciencias Astronómicas Astronomía galaxies:abundances ISM:abundances galaxies:nuclei
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/125393
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

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