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Polycyclic aromatic hydrocarbons and molecular hydrogen in oxygen-rich planetary nebulae: the case of NGC 6720

Evolved stars are primary sources for the formation of polycyclic aromatic hydrocarbons (PAHs) and dust grains. Their circumstellar chemistry is usually designated as either oxygen-rich or carbon-rich, although dual-dust chemistry objects, whose infrared spectra reveal both silicate- and carbon-dust...

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Detalhes bibliográficos
Publicado no:Mon Not R Astron Soc
Main Authors: Cox, N. L. J., Pilleri, P., Berné, O., Cernicharo, J., Joblin, C.
Formato: Artigo
Idioma:Inglês
Publicado em: 2016
Assuntos:
Acesso em linha:https://ncbi.nlm.nih.gov/pmc/articles/PMC4765080/
https://ncbi.nlm.nih.gov/pubmed/26924856
https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1093/mnrasl/slv184
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