Geer C P, Grossman S A
Johns Hopkins Oncology Center, Baltimore, MD 21287, USA.
J Neurooncol. 1997 May;32(3):193-201. doi: 10.1023/a:1005761031077.
High grade astrocytomas remain incurable even though these tumors often appear localized on modern imaging studies, rarely metastasize to systemic sites, and can be aggressively treated with surgery and radiation therapy. Recent data suggest that the dissemination of astrocytoma cells along white matter tracts to distant regions of the brain may be responsible for the poor survival of these patients and the limited impact of local therapies. Movement of astrocytoma cells along these white matter tracts can be active or passive in nature. To study the potential for tumor dissemination by bulk flow of interstitial fluid resulting from peritumoral edema. 20 microL of tritiated inulin, Evans Blue, and rat albumin were injected stereotactically into the right frontal lobe and the left temporal lobe at the gray-white matter junction in Sprague-Dawley rats. Six hours later, the rats were sacrificed and the brains were removed, frozen and prepared for quantitative autoradiography and histologic analysis. Interstitial flow rates were calculated from the autoradiographs, and flow pathways were determined from the movement of Evans Blue, inulin and histologic data. In each animal injected in the frontal lobe, Evans Blue and inulin were primarily confined to large ipsilateral white matter tracts and extended from the frontal injection site to the occipital lobe. The average interstitial fluid flow rate in the association fibers of the external capsule was 0.86 mm/hr. In contrast, the animals receiving temporal lobe injections had Evans Blue and inulin confined to the temporal lobe. The average interstitial fluid flow rate in the white matter tracts of the temporal lobe was 0.61 mm/hr. The rapid and preferential flow of interstitial fluid along white matter tracts and the differences in the clearance of extracellular fluid observed between the frontal and temporal lobes may have important clinical implications. These data suggest that aggressive treatment of peritumoral edema, expansion of radiotherapy ports, and consideration of the location of the tumor in treatment planning may improve therapeutic outcomes for some patients. An improved understanding of the mechanisms of tumor dissemination is crucial to designing more effective therapeutic approaches for patients with this devastating malignancy.
尽管高级别星形细胞瘤在现代影像学检查中通常表现为局限性,很少转移至全身部位,且可通过手术和放射治疗进行积极治疗,但它们仍然无法治愈。最近的数据表明,星形细胞瘤细胞沿白质束扩散至脑的远处区域可能是这些患者生存率低以及局部治疗效果有限的原因。星形细胞瘤细胞沿这些白质束的移动本质上可以是主动的或被动的。为了研究肿瘤周围水肿导致的间质液大量流动引起肿瘤播散的可能性,将20微升氚标记的菊粉、伊文思蓝和大鼠白蛋白立体定向注射到Sprague-Dawley大鼠右侧额叶和左侧颞叶的灰白质交界处。6小时后,处死大鼠并取出大脑,冷冻后准备进行定量放射自显影和组织学分析。根据放射自显影片计算间质流速,并根据伊文思蓝、菊粉的移动和组织学数据确定流动途径。在每只额叶注射的动物中,伊文思蓝和菊粉主要局限于同侧大的白质束,并从额叶注射部位延伸至枕叶。外囊联合纤维中的平均间质液流速为0.86毫米/小时。相比之下,接受颞叶注射的动物,伊文思蓝和菊粉局限于颞叶。颞叶白质束中的平均间质液流速为0.61毫米/小时。间质液沿白质束的快速和优先流动以及额叶和颞叶之间观察到的细胞外液清除差异可能具有重要的临床意义。这些数据表明,积极治疗肿瘤周围水肿、扩大放疗野以及在治疗计划中考虑肿瘤位置可能会改善一些患者的治疗效果。更好地理解肿瘤播散机制对于为患有这种毁灭性恶性肿瘤的患者设计更有效的治疗方法至关重要。