A light, scanning electron, and transmission electron microscopic study of pollen wall architecture in the subtribe Gnaphaliinae (Gnaphalieae, Asteraceae)

Abstract

To better understand relationships within the Asteroideae, the pollen morphology and exine structure of 10 genera and 15 species of Gnaphaliinae were investigated using light, scanning electron, and transmission electron microscopy. All taxa have a Gnaphalioid pattern of exine with an evidently rough foot layer. The tectal complex consists of three main layers that differ in morphology and thickness: a tectum, a median columellar layer, and an internal interlaced sub-columellar layer. The apertural system consists of an ectoaperture, a mesoaperture, and an endoaperture, which intersect, respectively, the tectal complex, the foot layer and the upper part of the endexine, and the inner part of the endexine. On the basis of pollen characteristics, especially those of the spines, all the species examined may be gathered into two groups, one including Helichrysum foetidum, H. italicum, Plecostachys serpyllifolia, and Pseudognaphalium luteo-album and the other including the other 11 species of Gnaphaliinae now investigated. In addition, because Gnaphalieae has been proposed as sister group to several tribes and clades of Asteroideae, a comparison was made between exine pattern in the Gnaphalieae and that in its putatively related tribes. On the basis of previous phylogenetic studies and our present pollen data we suggest that either Astereae, Astereae-Anthemideae clade, or Heliantheae s.l.-Anthemideae clade are the best candidates for the sister taxon/sister group of Gnaphalieae.