Antiarrhythmic effects of dichlorisoprenaline,H 56/28, ICI 50172, LB 46, MJ 1999 and propranolol on aconitine-induced atrial and ouabain-induced ventricular arrhythmias

Zusammenfassung Der Effekt von sechs-adrenergischen Blockierungsmitteln auf Akonitin-Arrhythmia bzw. Ouabain-Arrhythmia wurde mittels i.v. Verabreichung vergleichend untersucht. Reihenfolge der Wirksamkeit auf Akonitin-Arrhythmia: Propranolol>MJ 1999>LB 46>H 56/28, ICI 50172 und DCI, und dieselbe auf Ouabain-Arrhythmia: Propranolol, LB 46 und H 56/28 gleichwertig, MJ 1999 und ICI 50172 wirkungslos.     

Comparison ofβ-Adrenergic blocking activity of DCI,H56/28, ICI50172, LB46, methoxamine,MJ 1999 and propranolol in the blood perfused canine papillary muscle preparation

Zusammenfassung Nachweis, dass der-Blocker LB46 am blutperfundierten Papillarmuskel des Hundes eine grössere Aktivität aufweist als 6 andere bekannte-Blocker.     

Cloning and analysis of [NiFe]-hydrogenase genes from Arthrospira platensis FACHB341

0IntroductionHydrogenase(H2ase)has beeninvestigatedin a va-riety of bacterial groups since it was firstly reported in1931[1-3].Cyanobacteria contain two different types ofH2ase,uptake H2ase(EC1.12.7.2)and bidirectional orreversible H2ase(EC1.12.1.12).Uptake H2ase is in-duced under N2-fixing situation,mainly confinedin hete-rocysts.Bidirectional H2ase is constitutively synthesized,active in both heterocysts and vegetative cells present inboth N2-fixing and non-N2-fixing conditions.This en…     

The medaka draft genome and insights into vertebrate genome evolution

Teleosts comprise more than half of all vertebrate species and have adapted to a variety of marine and freshwater habitats. Their genome evolution and diversification are important subjects for the understanding of vertebrate evolution. Although draft genome sequences of two pufferfishes have been published, analysis of more fish genomes is desirable. Here we report a high-quality draft genome sequence of a small egg-laying freshwater teleost, medaka (Oryzias latipes). Medaka is native to East Asia and an excellent model system for a wide range of biology, including ecotoxicology, carcinogenesis, sex determination and developmental genetics. In the assembled medaka genome (700 megabases), which is less than half of the zebrafish genome, we predicted 20,141 genes, including approximately 2,900 new genes, using 5'-end serial analysis of gene expression tag information. We found single nucleotide polymorphisms (SNPs) at an average rate of 3.42% between the two inbred strains derived from two regional populations; this is the highest SNP rate seen in any vertebrate species. Analyses based on the dense SNP information show a strict genetic separation of 4 million years (Myr) between the two populations, and suggest that differential selective pressures acted on specific gene categories. Four-way comparisons with the human, pufferfish (Tetraodon), zebrafish and medaka genomes revealed that eight major interchromosomal rearrangements took place in a remarkably short period of approximately 50 Myr after the whole-genome duplication event in the teleost ancestor and afterwards, intriguingly, the medaka genome preserved its ancestral karyotype for more than 300 Myr.     

Long-term depressor effects of catecholamine neuronal grafts in the third ventricle of the brain in normotensive rats

Neuronal tissue containing A-6 group noradrenalin (NA) neurons of the locus ceruleus, or A-10 group dopamine (DA) neurons of the substantia nigra, was grafted into the third ventricle at the level of the preoptic-anterior hypothalamic region, in normotensive male rats. A significant and long-lasting depressor effect was shown in rats with either graft. In rats with an NA neuron-rich graft, plasma concentrations of arginine-vasopressin (AVP), plasma renin activity (PRA), and corticosterone (CS) decreased significantly, whereas in rats with a DA neuron-rich graft, AVP and PRA concentrations also decreased significantly but CS showed no significant change. Neither NA nor adrenalin in plasma changed significantly in rats with either graft.     

Identification of a major cytokinin in coconut milk

A major cytokinin found in coconut milk was isolted by using the tobacco callus growth-promoting assay as a guide during purification. The structure of the factor was determined to be 14-O-{3-O-[-d-galactopyranosyl-(12)--d--galactopyranosyl-(13)--L-arabinofuranosyl]-4-O-(-L-arabinofuranosyl)--d-galactopyranosyl}-trans-zeatin riboside [G₃A₂-ZR] by various NMR techniques, including heteronuclear multiple bond connectivity by 2D multiple quantum NMR (HMBC), as well as mass spectroscopy and sugar analysis. The optimum concentration of G₃A₂-ZR for cytokinin activity in the tobacco callus assay was estimated to be 5×10^–6 M, so that G₃A₂-ZR is one order of magnitude more potent than 1,3-diphenylurea and one order less potent than zeatin riboside. At least 20% of the cytokinin activity of coconut milk could be attributed to G₃A₂-ZR.     

Data model transformation in CAD system for multi-view modeling

This paper describes multi-view modeling and data model transformation for the modeling. We have proposed a reference model of CAD system generation, which can be applied to various domain-specific languages. However, the current CAD system generation cannot integrate data of multiple domains. Generally each domain has its own view of products. For example, in the domain of architectural structure, designers extract the necessary data from the data in architecture design. Domain experts translate one view into another view beyond domains using their own brains. The multi-view modeling is a way to integrate product data of multiple domains, and make it possible to translate views among various domains by computers.     

A galaxy at a redshift z = 6.96

When galaxy formation started in the history of the Universe remains unclear. Studies of the cosmic microwave background indicate that the Universe, after initial cooling (following the Big Bang), was reheated and reionized by hot stars in newborn galaxies at a redshift in the range 6 < z < 14 (ref. 1). Though several candidate galaxies at redshift z > 7 have been identified photometrically, galaxies with spectroscopically confirmed redshifts have been confined to z < 6.6 (refs 4-8). Here we report a spectroscopic redshift of z = 6.96 (corresponding to just 750 Myr after the Big Bang) for a galaxy whose spectrum clearly shows Lyman-alpha emission at 9,682 A, indicating active star formation at a rate of approximately 10M(o) yr(-1), where M(o) is the mass of the Sun. This demonstrates that galaxy formation was under way when the Universe was only approximately 6 per cent of its present age. The number density of galaxies at z approximately 7 seems to be only 18-36 per cent of the density at z = 6.6.