The population of planetary nebulae near the Galactic Centre: chemical abundances

Autor(es)

Cavichia, O. ; Costa, R. D. D. ; Maciel, W. J. ; Molla, M.

• Tipo de documento: Artigo Científico
• Fonte: Monthly Notices of the Royal Astronomical Society; v. 468, n. 1, p. 272-290, JUN 2017.
• Citações Web of Science: 3

Resumo

Planetary nebulae (PNe) constitute an important tool to study the chemical evolution of the Milky Way and other galaxies, probing the nucleosynthesis processes, abundance gradients and the chemical enrichment of the interstellar medium. In particular, Galactic bulge PNe (GBPNe) have been extensively used in the literature to study the chemical properties of this Galactic structure. However, the presently available GBPN chemical composition studies are strongly biased, since they were focused on brighter objects, predominantly located in Galactic regions of low interstellar reddening. In this work, we report physical parameters and abundances derived for a sample of 17 high-extinction PNe located in the inner 2 degrees of the Galactic bulge, based on low-dispersion spectroscopy secured at the Southern Astrophysical Research telescope using the Goodman spectrograph. The new data allow us to extend our data base including faint objects, providing chemical compositions for PNe located in this region of the bulge and an estimation for the masses of their progenitors to explore the chemical enrichment history of the central region of the Galactic bulge. The results show that there is an enhancement in the N/O abundance ratio in the Galactic Centre PNe compared with PNe located in the outer regions of the Galactic bulge. This may indicate recent episodes of star formation occurring near the Galactic Centre. (AU)

• Processo FAPESP: 07/07704-2 - Populações e evolução do bojo e região central da galáxia
• Beneficiário: Oscar Cavichia de Moraes
• Linha de fomento: Bolsas no Brasil - Doutorado
• Processo FAPESP: 10/18835-3 - Nebulosas planetárias, estrelas e evolução química de sistemas estelares
• Beneficiário: Roberto Dell'Aglio Dias da Costa
• Linha de fomento: Auxílio à Pesquisa - Temático
• Processo FAPESP: 12/01017-1 - Evolução química de galáxias espirais barradas e abundâncias químicas de nebulosas planetárias na direção central da Via Láctea
• Beneficiário: Oscar Cavichia de Moraes
• Linha de fomento: Bolsas no Brasil - Pós-Doutorado