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81.
Golgi biogenesis in Toxoplasma gondii 总被引:7,自引:0,他引:7
Pelletier L Stern CA Pypaert M Sheff D Ngô HM Roper N He CY Hu K Toomre D Coppens I Roos DS Joiner KA Warren G 《Nature》2002,418(6897):548-552
Two models have been put forward to explain the growth of new Golgi during the cell cycle. The first suggests that a new Golgi grows out of the endoplasmic reticulum by de novo synthesis. The second suggests that a pre-existing Golgi is needed for the growth of a new one, that is, the Golgi is an autonomously replicating organelle. To resolve this issue, we have exploited the simplicity of the apicomplexan parasite Toxoplasma gondii, which has only a single Golgi stack. Here we show, by using video fluorescence microscopy and three-dimensional reconstructions of serial thin sections, that the Golgi grows by a process of lateral extension followed by medial fission. Further fission leads to the inheritance by each daughter of a pair of Golgi structures, which then coalesce to re-form a single Golgi. Our results indicate that new Golgi grow by autonomous duplication and raise the possibility that the Golgi is a paired structure that is analogous to centrioles. 相似文献
82.
P. Stern Sabira Čatović N. Filipović 《Cellular and molecular life sciences : CMLS》1973,29(2):144-144
Summary Inhibition of glycine synthesis by aminopterine, an antagonist of pteroilglutaminic acid, causes rigidity of hind limbs in rats. This rigidity can be abolished by the injection of glycine. 相似文献
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P. Stern S. Huković M. Radivojević 《Cellular and molecular life sciences : CMLS》1976,32(10):1326-1327
Summary Synthetic Substance P and naloxone abolish the proconvulsive action of morphine on pentetrasol-induced seizures. It is suggested that Substance P could be a natural antagonist of morphine in the central nervous system.
Am 20. März 1976 gestorben. 相似文献
Am 20. März 1976 gestorben. 相似文献
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Taguchi A Blood DC del Toro G Canet A Lee DC Qu W Tanji N Lu Y Lalla E Fu C Hofmann MA Kislinger T Ingram M Lu A Tanaka H Hori O Ogawa S Stern DM Schmidt AM 《Nature》2000,405(6784):354-360
The receptor for advanced glycation end products (RAGE), a multi-ligand member of the immunoglobulin superfamily of cell surface molecules, interacts with distinct molecules implicated in homeostasis, development and inflammation, and certain diseases such as diabetes and Alzheimer's disease. Engagement of RAGE by a ligand triggers activation of key cell signalling pathways, such as p21ras, MAP kinases, NF-kappaB and cdc42/rac, thereby reprogramming cellular properties. RAGE is a central cell surface receptor for amphoterin, a polypeptide linked to outgrowth of cultured cortical neurons derived from developing brain. Indeed, the co-localization of RAGE and amphoterin at the leading edge of advancing neurites indicated their potential contribution to cellular migration, and in pathologies such as tumour invasion. Here we demonstrate that blockade of RAGE-amphoterin decreased growth and metastases of both implanted tumours and tumours developing spontaneously in susceptible mice. Inhibition of the RAGE-amphoterin interaction suppressed activation of p44/p42, p38 and SAP/JNK MAP kinases; molecular effector mechanisms importantly linked to tumour proliferation, invasion and expression of matrix metalloproteinases. 相似文献
90.
Stern D Eisenhardt P Spinrad H Dawson S van Breugel W Dey A de Vries W Stanford SA 《Nature》2000,408(6812):560-562
The identification of galaxies at extreme distances provides the most direct information about the earliest phases of galaxy formation. But at redshifts z > 5 even the most luminous galaxies appear faint; the interpretation of low signal-to-noise ratio data is difficult and misidentifications do occur. Here we report optical and near-infrared observations of the source STIS123627+621755, which was previously suggested to be at a redshift of 6.68 (ref. 1). At that redshift, and with the reported spectral energy distribution, the galaxy should be essentially invisible at wavelengths less than 9,300 A, because the intervening intergalactic medium absorbs almost all light energetic enough to ionize neutral hydrogen--that is, with wavelengths less than the redshifted Lyman limit of lambda = (1 + z) x 912A. At near-infrared wavelengths, however, the galaxy should be relatively bright. Here we report a detection of the galaxy at 6,700 A and a non-detection at a wavelength of 1.2 microm, contrary to expectations for z approximately 6.68. The data conservatively require that STIS123627+621755 has a redshift z < 6. 相似文献