Abundance determination in PNe: How to deal with large chemical inhomogeneities

Bibcode
2025IAUS..384..150M
DOI
10.1017/S1743921323005537
Morisset, C.; García-Rojas, J.; Gomez-Llanos, V.; Monteiro, H.
Referencia bibliográfica

IAU Symposium

Fecha de publicación:
0
2025
Número de autores
4
Número de autores del IAC
2
Número de citas
3
Número de citas referidas
0
Descripción
Abundance determinations in planetary nebulae (PNe) are crucial for understanding stellar evolution and the chemical evolution of the host galaxy. We discuss the complications involved when the presence of a metal-rich phase is suspected in the nebula. We demonstrate that the presence of a cold region emitting mainly metal recombination lines necessitates a detailed treatment to obtain an accurate assessment of the enrichment of this cold gas phase.
Tipo
Sin árbitro

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