Angiogenic properties of Kaposi's sarcoma-derived cells after long-term culture in vitro   总被引：31，自引：0，他引：31  

S Z Salahuddin  S Nakamura  P Biberfeld  M H Kaplan  P D Markham  L Larsson  R C Gallo 《Science (New York, N.Y.)》1988,242(4877):430-433

Cells derived from lung biopsies and pleural effusions from AIDS patients with Kaposi's sarcoma (KS) of the lungs were established in long-term culture with the aid of conditioned medium from HTLV-II-transformed T cells (HTLV-II CM). These AIDS-KS cells were similar to the so-called spindle cells in KS lesions and had some of their features. They produced factors that supported their own growth (autocrine) and the growth of other cells (paracrine), including umbilical vein endothelium and fibroblasts. That the AIDS-KS cells also expressed potent angiogenic activity was demonstrated by the chorioallantoic membrane assay and by subcutaneous inoculation of AIDS-KS cells into nude mice, which resulted in the development of angiogenic lesions composed of mouse cells and showing histological features similar to those of human KS lesions. These data suggest that AIDS-associated KS and possibly other types of KS may be initiated by signals that induce the growth of particular cells (spindle cells of lymphatic or vascular origin) and the expression of autocrine and paracrine activities.  相似文献   

Negative regulation of Wingless signaling by D-axin, a Drosophila homolog of axin     

Hamada F  Tomoyasu Y  Takatsu Y  Nakamura M  Nagai S  Suzuki A  Fujita F  Shibuya H  Toyoshima K  Ueno N  Akiyama T 《Science (New York, N.Y.)》1999,283(5408):1739-1742

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Crustal architecture of the cascadia forearc     

Trehu AM  Asudeh I  Brocher TM  Luetgert JH  Mooney WD  Nabelek JL  Nakamura Y 《Science (New York, N.Y.)》1994,266(5183):237-243

Seismic profiling data indicate that the thickness of an accreted oceanic terrane of Paleocene and early Eocene age, which forms the basement of much of the forearc beneath western Oregon and Washington, varies by approximately a factor of 4 along the strike of the Cascadia subduction zone. Beneath the Oregon Coast Range, the accreted terrane is 25 to 35 kilometers thick, whereas offshore Vancouver Island it is about 6 kilometers thick. These variations are correlated with variations in arc magmatism, forearc seismicity, and long-term forearc deformation. It is suggested that the strength of the forearc crust increases as the thickness of the accreted terrane increases and that the geometry of the seaward edge of this terrane influences deformation within the subduction complex and controls the amount of sediment that is deeply subducted.  相似文献   

Radon Anomaly: A Possible Precursor of the 1978 Izu-Oshima-kinkai Earthquake   总被引：1，自引：0，他引：1  

Wakita H  Nakamura Y  Notsu K  Noguchi M  Asada T 《Science (New York, N.Y.)》1980,207(4433):882-883

Precursory changes in the radon concentration of groundwater were observed prior to the Izu-Oshima-kinkai earthquake (magnitude 7.0) 14 January 1978. The distance from the epicenter to a continuous radon-monitoring station at Nakaizu was about 25 kilometers. A sudden drop and a subsequent increase in the radon concentration recorded on 9 January 1978 were significant. The size of the spike-like change was about 15 percent. After the earthquake, a remarkable increase in the radon concentration occurred.  相似文献   

Spherical bilayer vesicles of fullerene-based surfactants in water: a laser light scattering study     

Zhou S  Burger C  Chu B  Sawamura M  Nagahama N  Toganoh M  Hackler UE  Isobe H  Nakamura E 《Science (New York, N.Y.)》2001,291(5510):1944-1947

The low solubility of fullerenes in aqueous solution limits their applications in biology. By appropriate substitution, the fullerenes can be transformed into stabilized anions that are water soluble and can form large aggregated structures. A laser light scattering study of the association behavior of the potassium salt of pentaphenyl fullerene (Ph5C60K) in water revealed that the hydrocarbon anions Ph5C60- associate into bilayers, forming stable spherical vesicles with an average hydrodynamic radius and a radius of gyration of about 17 nanometers at a very low critical aggregation concentration of less than 10(-7) moles per liter. The average aggregation number of associated particles in these large spherical vesicles is about 1.2 x 10(4).  相似文献   

Seismic data from man-made impacts on the moon     

Latham G  Ewing M  Dorman J  Press F  Toksoz N  Sutton G  Meissner R  Duennebier F  Nakamura Y  Kovach R  Yates M 《Science (New York, N.Y.)》1970,170(3958):620-626

Unusually long reverberations were recorded from two lunar impacts by a seismic station installed on the lunar surface by the Apollo 12 astronauts. Seismic data from these impacts suggest that the lunar mare in the region of the Apollo 12 landing site consists of material with very low seismic velocities near the surface, with velocity increasing with depth to 5 to 6 kilometers per second (for compressional waves) at a depth of 20 kilometers. Absorption of seismic waves in this structure is extremely low relative to typical continental crustal materials on earth. It is unlikely that a major boundary similar to the crustmantle interface on earth exists in the outer 20 kilometers of the moon. A combination of dispersion and scattering of surface waves probably explains the lunar seismic reverberation. Scattering of these waves implies the presence of heterogeneity within the outer zone of the mare on a scale of from several hundred meters (or less) to several kilometers. Seismic signals from 160 events of natural origin have been recorded during the first 7 months of operation of the Apollo 12 seismic station. At least 26 of the natural events are small moonquakes. Many of the natural events are thought to be meteoroid impacts.  相似文献   

Cartilage acidic protein-1B (LOTUS), an endogenous Nogo receptor antagonist for axon tract formation     

Sato Y  Iketani M  Kurihara Y  Yamaguchi M  Yamashita N  Nakamura F  Arie Y  Kawasaki T  Hirata T  Abe T  Kiyonari H  Strittmatter SM  Goshima Y  Takei K 《Science (New York, N.Y.)》2011,333(6043):769-773

Neural circuitry formation depends on the molecular control of axonal projection during development. By screening with fluorophore-assisted light inactivation in the developing mouse brain, we identified cartilage acidic protein-1B as a key molecule for lateral olfactory tract (LOT) formation and named it LOT usher substance (LOTUS). We further identified Nogo receptor-1 (NgR1) as a LOTUS-binding protein. NgR1 is a receptor of myelin-derived axon growth inhibitors, such as Nogo, which prevent neural regeneration in the adult. LOTUS suppressed Nogo-NgR1 binding and Nogo-induced growth cone collapse. A defasciculated LOT was present in lotus-deficient mice but not in mice lacking both lotus- and ngr1. These findings suggest that endogenous antagonism of NgR1 by LOTUS is crucial for normal LOT formation.  相似文献   

Discovery of a Jupiter/Saturn analog with gravitational microlensing     

Gaudi BS  Bennett DP  Udalski A  Gould A  Christie GW  Maoz D  Dong S  McCormick J  Szymanski MK  Tristram PJ  Nikolaev S  Paczynski B  Kubiak M  Pietrzynski G  Soszynski I  Szewczyk O  Ulaczyk K  Wyrzykowski L;OGLE Collaboration  Depoy DL  Han C  Kaspi S  Lee CU  Mallia F  Natusch T  Pogge RW  Park BG;MuFUN Collaboration  Abe F  Bond IA  Botzler CS  Fukui A  Hearnshaw JB  Itow Y  Kamiya K  Korpela AV  Kilmartin PM  Lin W  Masuda K  Matsubara Y  Motomura M  Muraki Y  Nakamura S  Okumura T  Ohnishi K  Rattenbury NJ  Sako T  Saito T  Sato S 《Science (New York, N.Y.)》2008,319(5865):927-930

Searches for extrasolar planets have uncovered an astonishing diversity of planetary systems, yet the frequency of solar system analogs remains unknown. The gravitational microlensing planet search method is potentially sensitive to multiple-planet systems containing analogs of all the solar system planets except Mercury. We report the detection of a multiple-planet system with microlensing. We identify two planets with masses of approximately 0.71 and approximately 0.27 times the mass of Jupiter and orbital separations of approximately 2.3 and approximately 4.6 astronomical units orbiting a primary star of mass approximately 0.50 solar mass at a distance of approximately 1.5 kiloparsecs. This system resembles a scaled version of our solar system in that the mass ratio, separation ratio, and equilibrium temperatures of the planets are similar to those of Jupiter and Saturn. These planets could not have been detected with other techniques; their discovery from only six confirmed microlensing planet detections suggests that solar system analogs may be common.  相似文献   

Incipient space weathering observed on the surface of Itokawa dust particles     

Noguchi T  Nakamura T  Kimura M  Zolensky ME  Tanaka M  Hashimoto T  Konno M  Nakato A  Ogami T  Fujimura A  Abe M  Yada T  Mukai T  Ueno M  Okada T  Shirai K  Ishibashi Y  Okazaki R 《Science (New York, N.Y.)》2011,333(6046):1121-1125

The reflectance spectra of the most abundant meteorites, ordinary chondrites, are different from those of the abundant S-type (mnemonic for siliceous) asteroids. This discrepancy has been thought to be due to space weathering, which is an alteration of the surfaces of airless bodies exposed to the space environment. Here we report evidence of space weathering on particles returned from the S-type asteroid 25143 Itokawa by the Hayabusa spacecraft. Surface modification was found in 5 out of 10 particles, which varies depending on mineral species. Sulfur-bearing Fe-rich nanoparticles exist in a thin (5 to 15 nanometers) surface layer on olivine, low-Ca pyroxene, and plagioclase, which is suggestive of vapor deposition. Sulfur-free Fe-rich nanoparticles exist deeper inside (<60 nanometers) ferromagnesian silicates. Their texture suggests formation by metamictization and in situ reduction of Fe(2+).  相似文献   

Neutron activation analysis of a particle returned from asteroid Itokawa     

Ebihara M  Sekimoto S  Shirai N  Hamajima Y  Yamamoto M  Kumagai K  Oura Y  Ireland TR  Kitajima F  Nagao K  Nakamura T  Naraoka H  Noguchi T  Okazaki R  Tsuchiyama A  Uesugi M  Yurimoto H  Zolensky ME  Abe M  Fujimura A  Mukai T  Yada Y 《Science (New York, N.Y.)》2011,333(6046):1119-1121

A single grain (~3 micrograms) returned by the Hayabusa spacecraft was analyzed by neutron activation analysis. This grain is mainly composed of olivine with minor amounts of plagioclase, troilite, and metal. Our results establish that the Itokawa sample has similar chemical characteristics (iron/scandium and nickel/cobalt ratios) to chondrites, confirming that this grain is extraterrestrial in origin and has primitive chemical compositions. Estimated iridium/nickel and iridium/cobalt ratios for metal in the Itokawa samples are about five times lower than CI carbonaceous chondrite values. A similar depletion of iridium was observed in chondrule metals of ordinary chondrites. These metals must have condensed from the nebular where refractory siderophile elements already condensed and were segregated.  相似文献