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颗粒状角膜营养不良的异质性:TGFBI(BIGH3)基因中三个致病突变的鉴定——角膜淀粉样变性的经验教训

Heterogeneity in granular corneal dystrophy: identification of three causative mutations in the TGFBI (BIGH3) gene-lessons for corneal amyloidogenesis.

作者信息

Stewart H S, Ridgway A E, Dixon M J, Bonshek R, Parveen R, Black G

机构信息

Department of Medical Genetics and Regional Genetics Service, St Mary's Hospital, Manchester, UK.

出版信息

Hum Mutat. 1999;14(2):126-32. doi: 10.1002/(SICI)1098-1004(1999)14:2<126::AID-HUMU4>3.0.CO;2-W.

DOI:10.1002/(SICI)1098-1004(1999)14:2<126::AID-HUMU4>3.0.CO;2-W
PMID:10425035
Abstract

Six autosomal dominant corneal dystrophies are caused by mutations in the TGFBI (BIGH3) gene on chromosome 5q31: three types of lattice corneal dystrophy (LCD), including type I and type IIIA, granular, Avellino (ACD), and Reis-Bucklers. Initially an exact genotype-phenotype correlation was reported. We report three families, with differing clinical features, all presenting with "granular" corneal dystrophy. We analysed the TGFBI gene by SSCP analysis and direct sequencing in order to further assess the genotype-phenotype correlation. We describe three separate mutations in TGFBI: one novel, one initially described as causing ACD, and one previously described. The novel mutation, R124S, is at the identical position to the mutation causing LCD type I (CDL1). We review the clinical and histological phenotypes of the corneal dystrophies and hypothesize that the ability of a mutation to cause amyloid deposition depends on the location and nature of the mutation. In addition, we suggest that the classification of the granular corneal dystrophies be revised according to mutation type and that ACD should not be classified as a distinct morphological entity.

摘要

六种常染色体显性遗传性角膜营养不良是由位于5号染色体长臂31区的TGFBI(BIGH3)基因突变引起的:三种格子状角膜营养不良(LCD),包括I型和IIIA型、颗粒状、阿韦利诺(ACD)和Reis-Bucklers角膜营养不良。最初报道了确切的基因型-表型相关性。我们报告了三个临床特征不同但均表现为“颗粒状”角膜营养不良的家系。我们通过单链构象多态性分析(SSCP)和直接测序对TGFBI基因进行分析,以进一步评估基因型-表型相关性。我们描述了TGFBI基因中的三种不同突变:一种是新发现的,一种最初被描述为导致ACD的,还有一种是先前已描述的。新突变R124S与导致I型格子状角膜营养不良(CDL1)的突变位于相同位置。我们回顾了角膜营养不良的临床和组织学表型,并推测突变导致淀粉样沉积的能力取决于突变的位置和性质。此外,我们建议根据突变类型对颗粒状角膜营养不良进行重新分类,并且不应将ACD归类为一个独特的形态学实体。

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