A Tale of Two Tails: Untangling the Phylogeography and Demographic History of Extant Species of Mulgara (Dasycercus spp.) in the Australian Arid Zone

IF 3.6 2区 环境科学与生态学 Q2 ECOLOGY
Aline Gibson Vega, Brenton von Takach, Linette Umbrello, Dympna Cullen, Mark Cowan, Helen Crisp, Chris Dickman, Tim Doherty, William La Marca, Jenny Molyneux, Colleen Sims, Peter B. S. Spencer, Bobby Tamayo, Kym Ottewell
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Abstract

Aim

Australia's arid and semi-arid zones cover about 70% of the continent, yet our understanding of the biogeography of these diverse and expansive landscapes remains limited. Mulgara (Dasycercus spp.; Marsupialia: Dasyuridae), a widely distributed mammal taxon, offers an opportunity to explore patterns of the population structure across the region, previously hampered by taxonomic confusion surrounding extant species. Here, we aimed to (1) clarify the current distribution of extant Dasycercus lineages, (2) describe the population genomic structure of the widespread brush-tailed mulgara, and (3) determine whether observed patterns of population genomic structure in brush-tailed mulgara are consistent with biogeographic breaks.

Location

Arid and semi-arid regions of Australia.

Taxon

Two species are extant; the brush-tailed mulgara (D. blythi) and the crest-tailed mulgara (D. hillieri, previously D. cristicauda).

Methods

We sampled individuals from contemporary and museum tissue collections, obtaining next-generation sequencing data for 311 individuals, retaining 4360 single-nucleotide polymorphisms (SNPs) for population genomic analysis.

Results

We found that the two extant species are clearly delineated, corresponding well to current understanding of their respective distributions. The population genomic substructure in the brush-tailed mulgara (211 samples, 2740 SNPs) aligns primarily with major drainage divisions. Inference of historical population size change indicated that all populations have likely had stable population sizes for much of the past 1000 years, although post-European colonisation declines in some populations cannot be ruled out. The Pilbara population was most differentiated from other populations and displayed a stronger pattern of isolation-by-distance. Nevertheless, observed heterozygosity was similar across each of the populations (Ho = 0.078–0.090).

Conclusions

Stable population dynamics linked to the ecology of the mulgara and their high dispersal potential likely explain consistent levels of genetic diversity across most populations, but the effects of geography, such as major drainage divisions, drive the apparent contemporary population structure. Additional targeted tissue collection in under-sampled regions is recommended to better quantify genomic diversity, structure, and genetic health across the species' full range.

Abstract Image

两个尾巴的故事:解开澳大利亚干旱区现存Mulgara (Dasycercus spp.)物种的系统地理学和人口统计学历史
澳大利亚的干旱和半干旱地区约占大陆面积的70%,但我们对这些多样性和广阔景观的生物地理学理解仍然有限。Mulgara (Dasycercus spp.;有袋目:Dasyuridae)是一种分布广泛的哺乳动物分类单元,为探索该地区的种群结构模式提供了一个机会,以前由于现有物种的分类混乱而受到阻碍。在这里,我们的目的是(1)澄清现存的Dasycercus谱系的当前分布,(2)描述广泛分布的刷尾mulgara的群体基因组结构,以及(3)确定观察到的刷尾mulgara群体基因组结构模式是否与生物地理断裂相一致。地理位置:澳大利亚的干旱和半干旱地区。分类群现存两种;刷尾mulgara (D. blythi)和冠尾mulgara (D. hillieri,以前的D. cristicauda)。方法从当代和博物馆组织标本中采集个体样本,获得311个个体的下一代测序数据,保留4360个单核苷酸多态性(snp)用于群体基因组分析。结果两个现存的物种被清晰地描绘出来,与目前对它们各自分布的认识相吻合。211个样本中有2740个snp,刷尾狐猴种群基因组亚结构与主要的排水区基本一致。对历史人口规模变化的推断表明,在过去1000年的大部分时间里,所有人口的人口规模可能都保持稳定,尽管不能排除后欧洲殖民时期某些人口数量下降的可能性。皮尔巴拉种群与其他种群分化程度最高,表现出较强的距离隔离模式。然而,观察到的杂合度在每个群体中相似(Ho = 0.078 ~ 0.090)。结论稳定的种群动态与mulgara的生态环境及其高度的扩散潜力有关,这可能解释了大多数种群中遗传多样性的一致水平,但地理的影响,如主要的流域划分,驱动了明显的当代种群结构。建议在采样不足的地区收集额外的目标组织,以更好地量化整个物种的基因组多样性、结构和遗传健康。
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来源期刊
Journal of Biogeography
Journal of Biogeography 环境科学-生态学
CiteScore
7.70
自引率
5.10%
发文量
203
审稿时长
2.2 months
期刊介绍: Papers dealing with all aspects of spatial, ecological and historical biogeography are considered for publication in Journal of Biogeography. The mission of the journal is to contribute to the growth and societal relevance of the discipline of biogeography through its role in the dissemination of biogeographical research.
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