The tegument and associated structures of Haplometra cylindracea

Parasitology ◽  
1968 ◽  
Vol 58 (1) ◽  
pp. 1-7 ◽  
Author(s):  
L. T. Threadgold

The tegument of Haplometra cylindracea is protoplasmic. It is organized on two levels, a surface syncytium (‘cuticle’ of the light microscopists) and tegumental cells which lie among the parenchymal cells below the muscle layers. The surface syncytium and tegumental cells are joined together by protoplasmic, tube-like, processes.The surface syncytium is covered apically and basally by a unit plasma membrane. It contains mitochondria, vacuoles, lipid bodies, spines with a crystalline structure and dense secretory bodies. This syncytium lies on a basement membrane and a thick, fibrous, interstitial layer. The connecting protoplasmic processes, which originate from the base of the syncytium, are vacuolated and have few inclusions but, as they approach the tegumental cells, they become progressively filled with cytoplasm, cell inclusions and dense bodies.The tegumental cells consist of individual areas of nucleated protoplasm, usually lying in groups. These cells contain dense secretory bodies, mitochondria, a few lipid droplets, crystalline inclusions, and Golgi complexes. The Golgi complexes and granular endoplasmic reticulum are jointly involved in the production of a dense, probably proteinaceous, secretory body. Some qualitative regional differences in tegumental ultrastructure are described.The tegument of Haplometra is compared with that of other species so far described and like them must be considered both a protective and a secretory epithelium.I should like to express my sincere thanks to the following: The Wellcome Trust and Science Research Council for grants to purchase an Akashi TRS 50 and and A.E.I. EM6B electron microscope respectively; the Royal Society for a personal grant to purchase a Reichert Ultramicrotome and a vacuum coating unit; the Wellcome Trust for a grant to employ a Research Associate.

In April 1965 the Science Research Council received its Royal Charter and assumed responsibility for the support of major aspects of scientific research in the UK. This paper is primarily concerned with the consequent termination of the responsibility of the Royal Society for the Royal Greenwich Observatory and the subsequent cessation of the historic association of the Astronomer Royal with the Observatory. The Observatory was founded by King Charles II in 1675: see figure 1. The King’s advisers included Sir Jonas Moore, Surveyor-General of the Ordnance, who enlisted the help of John Flamsteed, a self-taught astronomer. The King appointed Flamsteed ‘our astronomical observator’ and through the historical accident that Moore was Flamsteed’s patron the Observatory came under the control of the Board of Ordnance. Although a number of Fellows of the Royal Society were involved in the recommendations for the founding of the Observatory, the Society had no formal responsibility for the Observatory or its work during the first 35 years of its existence. During those years Flamsteed’s relations with his contemporaries deteriorated, and the disputes, involving Halley and Newton, over the publication of his results, contributed to the issue of Queen Anne’s Warrant of 1710. By this Warrant the President of the Royal Society and other Fellows of the Society were appointed to serve as Visitors to the Observatory.


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