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21.
Nandkumar S. Shah L. E. Fox S. P. Martin 《Cellular and molecular life sciences : CMLS》1966,22(10):648-649
Zusammenfassung Bei den tuberkulösen Meerschweinchen wurde in der Niere eine erhöhte Aktivität der Glukose-6-Phosphatase beobachtet. Isoniazid hat die erhöhte Aktivität des Enzyms nicht erniedrigt, wenn es tuberkulösen Tieren vom 8. bis zum 38. Tage nach der Infektion oral verabreicht wurde. Es wird angenommen, dass die erhöhte Aktivität Ausdruck der Adaptionsfähigkeit von Glukose-6-Phosphatase ist.
Galesburg State Research Hospital, Galesburg, Illinois, USA. 相似文献
Galesburg State Research Hospital, Galesburg, Illinois, USA. 相似文献
22.
Zusammenfassung Eine morphologische Untersuchung des Vornierensystems in haploiden und diploiden Xenopuslarven weist darauf hin, dass das haploide Oedem nicht durch eine Funktionsstörung des Vornierensystems verursacht ist. 相似文献
23.
DNA uptake by a mutant strain of lymphoma cells 总被引:2,自引:0,他引:2
24.
An archaebacterial 5S rRNA contains a long insertion sequence 总被引:11,自引:0,他引:11
25.
Zusammenfassung Die zelluläre Reaktion an traumatischen, mechanisch gesetzten Läsionen in der Gehirnrinde wurde an neugeborenen und erwachsenen Hunden sowie an Mäusen untersucht. Die Heilung der Läsionen in Neugeborenen war so, dass das Gehirngewebe makroskopisch normal aussah; histologisch waren die durchtrennten Elemente durch die Heilungsprozesse unter minimaler glialer Reaktion wieder gut reorganisiert. 相似文献
26.
Numerous non-mammalian vertebrates have evolved lethal venoms to aid either in securing prey or as protection from predators, but modern mammals that use venoms in these ways are rare, including only the duck-billed platypus (Ornithorhynchus), the Caribbean Solenodon, and a few shrews (Soricidae) (Order Insectivora). Here we report evidence of a venom delivery apparatus in extinct mammals, documented by well-preserved specimens recovered from late Palaeocene rocks in Alberta, Canada. Although classified within Eutheria, these mammals are phylogenetically remote from modern Insectivora and have evolved specialized teeth as salivary venom delivery systems (VDSs) that differ markedly from one another and from those of Solenodon and shrews. Our discoveries therefore show that mammals have been much more flexible in the evolution of VDSs than previously believed, contradicting currently held notions that modern insectivorans are representative of the supposedly limited role of salivary venoms in mammalian history. Evidently, small predatory eutherians have paralleled colubroid snakes in evolving salivary venoms and their delivery systems several times independently. 相似文献
27.
28.
Page MJ Symeonidis M Vieira JD Altieri B Amblard A Arumugam V Aussel H Babbedge T Blain A Bock J Boselli A Buat V Castro-Rodríguez N Cava A Chanial P Clements DL Conley A Conversi L Cooray A Dowell CD Dubois EN Dunlop JS Dwek E Dye S Eales S Elbaz D Farrah D Fox M Franceschini A Gear W Glenn J Griffin M Halpern M Hatziminaoglou E Ibar E Isaak K Ivison RJ Lagache G Levenson L Lu N Madden S Maffei B Mainetti G Marchetti L Nguyen HT O'Halloran B Oliver SJ Omont A Panuzzo P Papageorgiou A 《Nature》2012,485(7397):213-216
The old, red stars that constitute the bulges of galaxies, and the massive black holes at their centres, are the relics of a period in cosmic history when galaxies formed stars at remarkable rates and active galactic nuclei (AGN) shone brightly as a result of accretion onto black holes. It is widely suspected, but unproved, that the tight correlation between the mass of the black hole and the mass of the stellar bulge results from the AGN quenching the surrounding star formation as it approaches its peak luminosity. X-rays trace emission from AGN unambiguously, whereas powerful star-forming galaxies are usually dust-obscured and are brightest at infrared and submillimetre wavelengths. Here we report submillimetre and X-ray observations that show that rapid star formation was common in the host galaxies of AGN when the Universe was 2-6 billion years old, but that the most vigorous star formation is not observed around black holes above an X-ray luminosity of 10(44) ergs per second. This suppression of star formation in the host galaxy of a powerful AGN is a key prediction of models in which the AGN drives an outflow, expelling the interstellar medium of its host and transforming the galaxy's properties in a brief period of cosmic time. 相似文献
29.
Haislip JB Nysewander MC Reichart DE Levan A Tanvir N Cenko SB Fox DB Price PA Castro-Tirado AJ Gorosabel J Evans CR Figueredo E MacLeod CL Kirschbrown JR Jelinek M Guziy S de Ugarte Postigo A Cypriano ES LaCluyze A Graham J Priddey R Chapman R Rhoads J Fruchter AS Lamb DQ Kouveliotou C Wijers RA Bayliss MB Schmidt BP Soderberg AM Kulkarni SR Harrison FA Moon DS Gal-Yam A Kasliwal MM Hudec R Vitek S Kubanek P Crain JA Foster AC Clemens JC Bartelme JW Canterna R Hartmann DH Henden AA Klose S 《Nature》2006,440(7081):181-183
Gamma-ray bursts (GRBs) and their afterglows are the most brilliant transient events in the Universe. Both the bursts themselves and their afterglows have been predicted to be visible out to redshifts of z approximately 20, and therefore to be powerful probes of the early Universe. The burst GRB 000131, at z = 4.50, was hitherto the most distant such event identified. Here we report the discovery of the bright near-infrared afterglow of GRB 050904 (ref. 4). From our measurements of the near-infrared afterglow, and our failure to detect the optical afterglow, we determine the photometric redshift of the burst to be z = 6.39 - 0.12 + 0.11 (refs 5-7). Subsequently, it was measured spectroscopically to be z = 6.29 +/- 0.01, in agreement with our photometric estimate. These results demonstrate that GRBs can be used to trace the star formation, metallicity, and reionization histories of the early Universe. 相似文献
30.
Soderberg AM Kulkarni SR Nakar E Berger E Cameron PB Fox DB Frail D Gal-Yam A Sari R Cenko SB Kasliwal M Chevalier RA Piran T Price PA Schmidt BP Pooley G Moon DS Penprase BE Ofek E Rau A Gehrels N Nousek JA Burrows DN Persson SE McCarthy PJ 《Nature》2006,442(7106):1014-1017
Over the past decade, long-duration gamma-ray bursts (GRBs)--including the subclass of X-ray flashes (XRFs)--have been revealed to be a rare variety of type Ibc supernova. Although all these events result from the death of massive stars, the electromagnetic luminosities of GRBs and XRFs exceed those of ordinary type Ibc supernovae by many orders of magnitude. The essential physical process that causes a dying star to produce a GRB or XRF, and not just a supernova, is still unknown. Here we report radio and X-ray observations of XRF 060218 (associated with supernova SN 2006aj), the second-nearest GRB identified until now. We show that this event is a hundred times less energetic but ten times more common than cosmological GRBs. Moreover, it is distinguished from ordinary type Ibc supernovae by the presence of 10(48) erg coupled to mildly relativistic ejecta, along with a central engine (an accretion-fed, rapidly rotating compact source) that produces X-rays for weeks after the explosion. This suggests that the production of relativistic ejecta is the key physical distinction between GRBs or XRFs and ordinary supernovae, while the nature of the central engine (black hole or magnetar) may distinguish typical bursts from low-luminosity, spherical events like XRF 060218. 相似文献