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通过一种算法对培养星形胶质细胞中的丝状伪足进行定量分析。

Quantifying Filopodia in Cultured Astrocytes by an Algorithm.

作者信息

Aumann Georg, Friedländer Felix, Thümmler Matthias, Keil Fabian, Brunkhorst Robert, Korf Horst-Werner, Derouiche Amin

机构信息

Institute of Anatomy, University of Dresden, Dresden, Germany.

Hospital of Günzburg, Günzburg, Germany.

出版信息

Neurochem Res. 2017 Jun;42(6):1795-1809. doi: 10.1007/s11064-017-2193-0. Epub 2017 Feb 27.

Abstract

Astrocytes in vivo extend thin processes termed peripheral astrocyte processes (PAPs), in particular around synapses where they can mediate glia-neuronal communication. The relation of PAPs to synapses is not based on coincidence, but it is not clear which stimuli and mechanisms lead to their formation and are active during process extension/ retraction in response to neuronal activity. Also, the molecular basis of the extremely fine PAP morphology (often 50 to 100 nm) is not understood. These open questions can be best investigated under in vitro conditions studying glial filopodia. We have previously analyzed filopodial mechanisms (Lavialle et al. PNAS 108:12915) applying an automated method for filopodia morphometry, which is now described in greater detail. The Filopodia Specific Shape Factor (FSSF) developed integrates number and length of filopodia. It quantifies filopodia independent of overall astrocytic shape or size, which can be intricate in itself. The algorithm supplied here permits automated image processing and measurements using ImageJ. Cells have to be sampled in higher numbers to obtain significant results. We validate the FSSF, and characterize the systematic influence of thresholding and camera pixel grid on measurements. We provide exemplary results of substance-induced filopodia dynamics (glutamate, mGluR agonists, EGF), and show that filopodia formation is highly sensitive to medium pH (CO) and duration of cell culture. Although the FSSF was developed to study astrocyte filopodia with focus on the perisynaptic glial sheath, we expect that this parameter can also be applied to neuronal growth cones, non-neural cell types, or cell lines.

摘要

在体内,星形胶质细胞会伸出称为外周星形胶质细胞突起(PAPs)的细突起,特别是在突触周围,它们可介导神经胶质-神经元通讯。PAPs与突触的关系并非基于巧合,但尚不清楚哪些刺激和机制导致其形成,以及在响应神经元活动的突起延伸/回缩过程中哪些机制是活跃的。此外,对于极其纤细的PAP形态(通常为50至100纳米)的分子基础也尚不明确。这些悬而未决的问题在体外研究神经胶质丝状伪足的条件下能够得到最佳研究。我们之前已运用一种用于丝状伪足形态测量的自动化方法分析了丝状伪足机制(拉维阿勒等人,《美国国家科学院院刊》108:12915),现在将对此进行更详细的描述。所开发的丝状伪足特定形状因子(FSSF)整合了丝状伪足的数量和长度。它能独立于星形胶质细胞的整体形状或大小对丝状伪足进行量化,而星形胶质细胞自身的整体形状或大小可能很复杂。此处提供的算法允许使用ImageJ进行自动化图像处理和测量。必须对更多细胞进行采样以获得显著结果。我们验证了FSSF,并表征了阈值设定和相机像素网格对测量的系统性影响。我们提供了物质诱导的丝状伪足动力学(谷氨酸、代谢型谷氨酸受体激动剂、表皮生长因子)的示例性结果,并表明丝状伪足的形成对培养基pH值(二氧化碳)和细胞培养持续时间高度敏感。尽管FSSF是为研究围绕突触周围神经胶质鞘的星形胶质细胞丝状伪足而开发的,但我们预计该参数也可应用于神经元生长锥、非神经细胞类型或细胞系。

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