Chemical abundances of planetary nebulae in the substructures of M31 : II. The extended sample and a comparison study with the Outer-disk Group

We report deep spectroscopy of 10 planetary nebulae (PNe) in the Andromeda Galaxy (M31) using the 10.4 m Gran Telescopio Canarias (GTC). Our targets reside in different regions of M31, including halo streams and the dwarf satellite M32, and kinematically deviate from the extended disk. The temperatu...

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Detalles Bibliográficos
Autores principales:	Fang, Xuan, García Benito, Rubén, Guerrero, Martín A., Zhang, Yong, Liu, Xiaowei, Morisset, Christophe, Karakas, Amanda I., Miller Bertolami, Marcelo Miguel, Yuan, Haibo, Cabrera Lavers, Antonio
Formato:	Articulo
Lenguaje:	Inglés
Publicado:	2018
Materias:	Astronomía galaxies: abundances galaxies: evolution galaxies: individual (M31) ISM: abundances planetary nebulae: general stars: evolution
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/93569 https://iopscience.iop.org/0004-637X/853/1/50/ https://ri.conicet.gov.ar/handle/11336/82602
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

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