Forbes D P, Steffek A J, Klepacki M
Department of Orthodontics, Northwestern University Dental School, Chicago, Illinois 60611.
J Craniofac Genet Dev Biol. 1989;9(3):271-83.
The epithelial surfaces of the facial primordia were evaluated by scanning electron microscopy (SEM) during primary palatogenesis in two genetically related mouse strains, the A/J and the A/WySn strains. These two strains were selected because the reported frequency of spontaneous cleft lip with or without cleft palate [CL(P)] in the A/J strain approximates 0%, whereas the spontaneous frequency of CL(P) in the A/WySn strain is 20-30%. The embryos were examined prior to (two to six tail somites), during (seven to ten tail somites), and after (ten to 14 tail somites) primary palate fusion. During fusion, epithelial surface activity (characterized as cellular debris, dissociated cells, cellular projections, and epithelial bridging) was more pronounced in A/J embryos. A/WySn embryos with spontaneous cleft lip exhibited a marked deficiency in epithelial activity when compared to their normal littermates. No discernible differences were detected in the facial morphology, with the exception of the distal end of the medial nasal prominence, which appeared longer in the A/J strain. This study suggests that the degree of epithelial surface activity at the putative site of fusion and the relative length of the medial nasal prominence may account for the observed differences in facial clefting of the two strains. Face shape, related to prominence divergence, was similar in the two strains and could not explain the higher incidence of clefting observed in the A/WySn strain.
在两个具有遗传关系的小鼠品系A/J和A/WySn的原发性腭形成过程中,通过扫描电子显微镜(SEM)对颜面原基的上皮表面进行了评估。选择这两个品系是因为据报道,A/J品系中伴有或不伴有腭裂的唇裂[CL(P)]自发频率约为0%,而A/WySn品系中CL(P)的自发频率为20%-30%。在原发性腭融合之前(2至6个尾节)、期间(7至10个尾节)和之后(10至14个尾节)对胚胎进行检查。在融合过程中,上皮表面活性(表现为细胞碎片、解离细胞、细胞突起和上皮桥接)在A/J胚胎中更为明显。与正常同窝仔相比,患有自发唇裂的A/WySn胚胎在上皮活性方面存在明显缺陷。除了内侧鼻突的远端在A/J品系中显得更长外,在面部形态上未检测到明显差异。这项研究表明,融合假定部位的上皮表面活性程度以及内侧鼻突的相对长度可能是导致这两个品系面部裂隙差异的原因。与突出差异相关的面部形状在两个品系中相似,无法解释在A/WySn品系中观察到的更高的裂隙发生率。