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111.
本文用自制板框式电解槽对电解还原制备L-半胱氨酸盐酸盐的工艺条件,如电解终止时间的判断、电极、电解质溶液、隔膜……等进行了一系列的选择和研究。特别是采用电解液外循环工艺,研究了循环流速对电解还原速度的影响,以及流速和电流密度等诸因素的关系。 相似文献
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本文报告1例罕见的肾钙乳沉积症,本症是肾盂源性囊肿内有钙乳沉积,分为两类;第一类,钙乳沉积于扩大的肾盂源性囊肿内,肾功能正常,占多数;第二类,有明显的肾积水和肾盏扩张,合并多发性钙乳沉积,肾功能差,属少数。病理检查,肾囊肿囊壁有肾单位存在,估计是由于集合管梗阻而形成的囊肿,经年累月接受其所属肾单位分泌的微量尿液,在浓缩功能差的情况下,潴留囊肿内的晶体便保持糊状微粒状态。本例钙乳沉积物的化学分析表明,其成份含有9种元素,其中以钙、铝、硅、及镁含量最多。x线检查的特征性图像是诊断本症的主要方法。囊肿去盖术对本症是一种安全而有效的术式。 相似文献
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C. Loštický 《Cellular and molecular life sciences : CMLS》1969,25(10):1034-1034
Zusammenfassung Es wurden Interaktionen von Protamin mit vorher in Agar-Gel elektrophoretisch getrennten plasmatischen Eiweisskörpern untersucht. Neben der schon früher bekannten Interaktion mit Fibrinogen wurden auch solche mit beiden Klassen der plasmatischen Lipoproteine gefunden. 相似文献
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The breast cancer susceptibility protein BRCA2 controls the function of RAD51, a recombinase enzyme, in pathways for DNA repair by homologous recombination. We report here the structure of a complex between an evolutionarily conserved sequence in BRCA2 (the BRC repeat) and the RecA-homology domain of RAD51. The BRC repeat mimics a motif in RAD51 that serves as an interface for oligomerization between individual RAD51 monomers, thus enabling BRCA2 to control the assembly of the RAD51 nucleoprotein filament, which is essential for strand-pairing reactions during DNA recombination. The RAD51 oligomerization motif is highly conserved among RecA-like recombinases, highlighting a common evolutionary origin for the mechanism of nucleoprotein filament formation, mirrored in the BRC repeat. Cancer-associated mutations that affect the BRC repeat disrupt its predicted interaction with RAD51, yielding structural insight into mechanisms for cancer susceptibility. 相似文献
119.
VEGFR1-positive haematopoietic bone marrow progenitors initiate the pre-metastatic niche 总被引:4,自引:0,他引:4
Kaplan RN Riba RD Zacharoulis S Bramley AH Vincent L Costa C MacDonald DD Jin DK Shido K Kerns SA Zhu Z Hicklin D Wu Y Port JL Altorki N Port ER Ruggero D Shmelkov SV Jensen KK Rafii S Lyden D 《Nature》2005,438(7069):820-827
The cellular and molecular mechanisms by which a tumour cell undergoes metastasis to a predetermined location are largely unknown. Here we demonstrate that bone marrow-derived haematopoietic progenitor cells that express vascular endothelial growth factor receptor 1 (VEGFR1; also known as Flt1) home to tumour-specific pre-metastatic sites and form cellular clusters before the arrival of tumour cells. Preventing VEGFR1 function using antibodies or by the removal of VEGFR1(+) cells from the bone marrow of wild-type mice abrogates the formation of these pre-metastatic clusters and prevents tumour metastasis, whereas reconstitution with selected Id3 (inhibitor of differentiation 3)-competent VEGFR1+ cells establishes cluster formation and tumour metastasis in Id3 knockout mice. We also show that VEGFR1+ cells express VLA-4 (also known as integrin alpha4beta1), and that tumour-specific growth factors upregulate fibronectin--a VLA-4 ligand--in resident fibroblasts, providing a permissive niche for incoming tumour cells. Conditioned media obtained from distinct tumour types with unique patterns of metastatic spread redirected fibronectin expression and cluster formation, thereby transforming the metastatic profile. These findings demonstrate a requirement for VEGFR1+ haematopoietic progenitors in the regulation of metastasis, and suggest that expression patterns of fibronectin and VEGFR1+VLA-4+ clusters dictate organ-specific tumour spread. 相似文献
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Although it is widely accepted that most galaxies have supermassive black holes at their centres, concrete proof has proved elusive. Sagittarius A* (Sgr A*), an extremely compact radio source at the centre of our Galaxy, is the best candidate for proof, because it is the closest. Previous very-long-baseline interferometry observations (at 7 mm wavelength) reported that Sgr A* is approximately 2 astronomical units (au) in size, but this is still larger than the 'shadow' (a remarkably dim inner region encircled by a bright ring) that should arise from general relativistic effects near the event horizon of the black hole. Moreover, the measured size is wavelength dependent. Here we report a radio image of Sgr A* at a wavelength of 3.5 mm, demonstrating that its size is approximately 1 au. When combined with the lower limit on its mass, the lower limit on the mass density is 6.5 x 10(21)M(o) pc(-3) (where M(o) is the solar mass), which provides strong evidence that Sgr A* is a supermassive black hole. The power-law relationship between wavelength and intrinsic size (size proportional, variantwavelength(1.09)) explicitly rules out explanations other than those emission models with stratified structure, which predict a smaller emitting region observed at a shorter radio wavelength. 相似文献