Astrocytic contributions to Huntington's disease pathophysiology

Publikation: Bidrag til tidsskriftReviewForskningfagfællebedømt

Huntington's disease (HD) is a fatal, monogenic, autosomal dominant neurodegenerative disease caused by a polyglutamine-encoding CAG expansion in the huntingtin (HTT) gene that results in mutant huntingtin proteins (mHTT) in cells throughout the body. Although large parts of the central nervous system (CNS) are affected, the striatum is especially vulnerable and undergoes marked atrophy. Astrocytes are abundant within the striatum and contain mHTT in HD, as well as in mouse models of the disease. We focus on striatal astrocytes and summarize how they participate in, and contribute to, molecular pathophysiology and disease-related phenotypes in HD model mice. Where possible, reference is made to pertinent astrocyte alterations in human HD. Astrocytic dysfunctions related to cellular morphology, extracellular ion and neurotransmitter homeostasis, and metabolic support all accompany the development and progression of HD, in both transgenic mouse and human cellular and chimeric models of HD. These findings reveal the potential for the therapeutic targeting of astrocytes so as to restore synaptic as well as tissue homeostasis in HD. Elucidation of the mechanisms by which astrocytes contribute to HD pathogenesis may inform a broader understanding of the role of glial pathology in neurodegenerative disorders and, by so doing, enable new strategies of glial-directed therapeutics.
OriginalsprogEngelsk
TidsskriftAnnals of the New York Academy of Sciences
Vol/bind1522
Udgave nummer1
Sider (fra-til)42-59
Antal sider18
ISSN0077-8923
DOI
StatusUdgivet - 2023

Bibliografisk note

Funding Information:
HD work in the Khakh lab was supported by CHDI Inc. and by NIH grant R35NS111583. Work discussed from the Goldman lab was supported by the Lundbeckfonden, the Novo Nordisk Foundation, and the Adel-son Medical Research Foundation; past studies were also funded by CHDI. The authors regret that many papers could not be cited, because of space limits and the focus on studies from the last 5 years. B.S.K. is grateful to members of his lab, Vahri Beaumont, Roger Cachope, and Ignacio Munoz-Sanjuan for discussions over the last 10 years.

Funding Information:
HD work in the Khakh lab was supported by CHDI Inc. and by NIH grant R35NS111583. Work discussed from the Goldman lab was supported by the Lundbeckfonden, the Novo Nordisk Foundation, and the Adelson Medical Research Foundation; past studies were also funded by CHDI. The authors regret that many papers could not be cited, because of space limits and the focus on studies from the last 5 years. B.S.K. is grateful to members of his lab, Vahri Beaumont, Roger Cachope, and Ignacio Munoz-Sanjuan for discussions over the last 10 years.

Publisher Copyright:
© 2023 New York Academy of Sciences.

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