3′–5′-cAMP and lysosome membrane labilization

Zusammenfassung Es wird gezeigt, dass 3–5-cAMP (10^–3 M) und Theophyllin (10^–4 M) die Permeabilität derjenigen Lysosmen-Membranen steigern, die aus Rattenleberzellen in bezug auf saure Phosphatase and in bezug auf -Glucuronidase-Enzyme präpariert wurden.     

Der Übertritt von Antikörpern gegen Nahrungsmittel-Antigene in die Frauenmilch

Summary In a high percentage of lactating mothers the presence of antibodies against cow's milk could be shown in breast milk by means of the hemagglutination test. This passage does not appear to be continuous. Possible implications of these findings with respect to the pathogenesis of Ablactation-Dyspepsia are discussed.

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Für die technische Hilfe bei den Untersuchungen sind wir FräuleinA. Sauer schr zu Dank verpflichtet.     

Vagus pneumonia as membrane phospholipase activation

Zusammenfassung Die relative Abnahme des Phospholipid-Gehalts und das erhöhte Niveau des FFA weist auf eine Phospholipase-Aktivität nach Vagotomie hin. Diese Befunde können durch Propranolol gehemmt werden.     

Discovery of radio emission from the brown dwarf LP944-20

Brown dwarfs are not massive enough to sustain thermonuclear fusion of hydrogen at their centres, but are distinguished from gas-giant planets by their ability to burn deuterium. Brown dwarfs older than approximately 10 Myr are expected to possess short-lived magnetic fields and to emit radio and X-rays only very weakly from their coronae. An X-ray flare was recently detected on the brown dwarf LP944-20, whereas previous searches for optical activity (and one X-ray search) yielded negative results. Here we report the discovery of quiescent and flaring radio emission from LP944-20, with luminosities several orders of magnitude larger than predicted by the empirical relation between the X-ray and radio luminosities that has been found for many types of stars. Interpreting the radio data within the context of synchrotron emission, we show that LP944-20 has an unusually weak magnetic field in comparison to active M-dwarf stars, which might explain the previous null optical and X-ray results, as well as the strength of the radio emissions compared to those at X-ray wavelengths.