Chromosome-wide distribution of haplotype blocks and the role of recombination hot spots

被引:224
作者
Phillips, MS
Lawrence, R
Sachidanandam, R
Morris, AP
Balding, DJ
Donaldson, MA
Studebaker, JF
Ankener, WM
Alfisi, SV
Kuo, FS
Camisa, AL
Pazorov, V
Scott, KE
Carey, BJ
Faith, J
Katari, G
Bhatti, HA
Cyr, JM
Derohannessian, V
Elosua, C
Forman, AM
Grecco, NM
Hock, CR
Kuebler, JM
Lathrop, JA
Mockler, MA
Nachtman, EP
Restine, SL
Varde, SA
Hozza, MJ
Gelfand, CA
Broxholme, J
Abecasis, GR
Boyce-Jacino, MT
Cardon, LR
机构
[1] Univ Oxford, Wellcome Trust Ctr Human Genet, Oxford OX3 7BN, England
[2] Orchid Biosci Inc, Princeton, NJ 08540 USA
[3] Cold Spring Harbor Lab, Cold Spring Harbor, NY 11724 USA
[4] Univ London Imperial Coll Sci Technol & Med, Dept Epidemiol & Publ Hlth, Fac Med, London W2 1PG, England
[5] Univ Michigan, Ann Arbor, MI 48109 USA
基金
英国惠康基金;
关键词
D O I
10.1038/ng1100
中图分类号
Q3 [遗传学];
学科分类号
071007 ; 090102 ;
摘要
Recent studies of human populations suggest that the genome consists of chromosome segments that are ancestrally conserved ('haplotype blocks'; refs. 1-3) and have discrete boundaries defined by recombination hot spots(4,5). Using publicly available genetic markers(6), we have constructed a first-generation haplotype map of chromosome 19. As expected for this marker density(7), approximately one-third of the chromosome is encompassed within haplotype blocks. Evolutionary modeling of the data indicates that recombination hot spots are not required to explain most of the observed blocks, providing that marker ascertainment and the observed marker spacing are considered. In contrast, several long blocks are inconsistent with our evolutionary models, and different mechanisms could explain their origins.
引用
收藏
页码:382 / 387
页数:6
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