Abstract
This paper reviews the various processes that have been proposed to explain the observed trend of PAH strength with metallicity. It summarizes a study showing that, although PAH destruction by hard radiation is important in low-metallicity environments, it is not sufficient to explain their paucity. In these systems, the deficiency of their formation mechanism, related to stellar evolution, has to be invoked. © EAS, EDP Sciences 2011.
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CITATION STYLE
APA
Galliano, F. (2011). Dialectics of the PAH abundance trend with metallicity. In EAS Publications Series (Vol. 46, pp. 43–48). https://doi.org/10.1051/eas/1146004
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