Biosynthesis of alkaloids. On the occurrence of keto acids inPapaver somniferum L. Plants

Zusammenfassung BeiPapaver somniferum L. wurde im Laufe der Ontogenese die Anwesenheit von Ketosäuren des Zitronensäurecyclus verfolgt. Zur Blütezeit und nach dem Verblühen konnten auch die aromatischen Ketosäuren, Phenylbrenztraubensäure undp-Hydroxyphenylbrenztraubensäure nachgewiesen werden (2,4-Dinitrophenylhydrazone und nach Reduktion zu Aminosäuren: Phenylalanin und Tyrosin).     

Studies on the hypoglycemic effect of ‘Vincamin’

Zusammenfassung Nach Verabreichung von Vincamin sinkt bei akuten Versuchen an Ratten der Blutzuckerspiegel. Die nach Dextroseverfütterung verursachte Hyperglykämie wird durch Vincamin verhindert, der Blutzuckeranstieg jedoch bleibt nach Adrenalin unbeeinflusst.     

Possible in situ formation of meteoritic nanodiamonds in the early Solar System

Grains of dust that pre-date the Sun provide insights into their formation around other stars and into the early evolution of the Solar System. Nanodiamonds recovered from meteorites, which originate in asteroids, have been thought to be the most abundant type of presolar grain. If that is true, then nanodiamonds should be at least as abundant in comets, because they are thought to have formed further out in the early Solar System than the asteroid parent bodies, and because they should be more pristine. Here we report that nanodiamonds are absent or very depleted in fragile, carbon-rich interplanetary dust particles, some of which enter the atmosphere at speeds within the range of cometary meteors. One interpretation of the results is that some (perhaps most) nanodiamonds formed within the inner Solar System and are not presolar at all, consistent with the recent detection of nanodiamonds within the accretion discs of other young stars. An alternative explanation is that all meteoritic nanodiamonds are indeed presolar, but that their abundance decreases with heliocentric distance, in which case our understanding of large-scale transport and circulation within the early Solar System is incomplete.     

Detecting recent positive selection in the human genome from haplotype structure

The ability to detect recent natural selection in the human population would have profound implications for the study of human history and for medicine. Here, we introduce a framework for detecting the genetic imprint of recent positive selection by analysing long-range haplotypes in human populations. We first identify haplotypes at a locus of interest (core haplotypes). We then assess the age of each core haplotype by the decay of its association to alleles at various distances from the locus, as measured by extended haplotype homozygosity (EHH). Core haplotypes that have unusually high EHH and a high population frequency indicate the presence of a mutation that rose to prominence in the human gene pool faster than expected under neutral evolution. We applied this approach to investigate selection at two genes carrying common variants implicated in resistance to malaria: G6PD and CD40 ligand. At both loci, the core haplotypes carrying the proposed protective mutation stand out and show significant evidence of selection. More generally, the method could be used to scan the entire genome for evidence of recent positive selection.