Planetary nebulae in the Small Magellanic Cloud

Planetary nebulae in the Small Magellanic Cloud

We analyse the planetary nebulae (PNe) population of the Small Magellanic Cloud (SMC), based on evolutionary models of stars with metallicities in the range 10−3 ≤ Z ≤ 4 × 10−3 and mass 0.9 M⊙ 

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Bibliographische Detailangaben
Veröffentlicht in:Monthly notices of the Royal Astronomical Society 2016-08, Vol.460 (4), p.3940-3949
Hauptverfasser: Ventura, P., Stanghellini, L., Di Criscienzo, M., García-Hernández, D. A., Dell'Agli, F.
Format: Artikel
Sprache:eng
Schlagworte:
Astronomy
Asymptotic properties
Chemical composition
Combustion
Comparative analysis
Evolution
Evolutionary
Magellanic clouds
Nebulae
Planetary nebulae
Star & galaxy formation
Stars
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Beschreibung
Zusammenfassung:We analyse the planetary nebulae (PNe) population of the Small Magellanic Cloud (SMC), based on evolutionary models of stars with metallicities in the range 10−3 ≤ Z ≤ 4 × 10−3 and mass 0.9 M⊙ 
ISSN:0035-8711
1365-2966
DOI:10.1093/mnras/stw1254