Walsh & Hoyt: Astrocytic Tumors

Update Item Information
Identifier wh_ch29_p1415_2
Title Walsh & Hoyt: Astrocytic Tumors
Creator Thomas R. Hedges III, MD
Affiliation New England Eye Center
Subject Neurology; Ophthalmology; Eye Diseases; Astrocytic Tumors
Description Astrocytes can be separated based on their histologic appearance into two main types: fibrillary and protoplasmic. Fibrillary astrocytes are present throughout the central nervous system (CNS) except in gray matter, where protoplasmic astrocytes predominate. Fibrillary astrocytes contain fine fibers in their cell bodies and processes, whereas protoplasmic astrocytes have only a few such fibers that are seen only with electron microscopy. The nuclei of fibrillary astrocytes are irregular in shape and contain numerous indentations, whereas the nuclei of protoplasmic astrocytes are round or ovoid and have a smooth outline. The processes of fibrillary astrocytes, some of which make contact with capillaries and others with pia mater, are smooth, long, and branch freely, and those of protoplasmic astrocytes are irregular and have fewer branches. These histologic differences help distinguish the two types of astrocytes, particularly when they are examined in sections stained with gold-mercury or silver impregnation.
Date 2005
Language eng
Format application/pdf
Type Text
Source Walsh and Hoyt's Clinical Neuro-Ophthalmology, 6th Edition
Relation is Part of Walsh and Hoyt's Clinical Neuro-Ophthalmology Walsh and Hoyt's Clinical Neuro-Ophthalmology
Collection Neuro-ophthalmology Virtual Education Library: NOVEL http://NOVEL.utah.edu
Publisher Wolters Kluwer Health, Philadelphia
Holding Institution Spencer S. Eccles Health Sciences Library, University of Utah, 10 N 1900 E SLC, UT 84112-5890
Rights Management Copyright 2005. For further information regarding the rights to this collection, please visit: https://NOVEL.utah.edu/about/copyright
ARK ark:/87278/s66h7rvh
Setname ehsl_novel_whts
ID 186044
Reference URL https://collections.lib.utah.edu/ark:/87278/s66h7rvh
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