Testing of rifampicin on possible genetic effects onDrosophila melanogaster and human leukocyte chromosomes in vitro

Zusammenfassung Mutagenitätsuntersuchungen von Rifampicin anDrosophila melanogas (X-chromosomale rezessive Letalmutationen) und an menschlichen Leukozytenchromosomen in vitro ergaben keine Anhaltspunkte für eine genetische Wirksamkeit dieser Substanz.

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We thank Mrs.R. Pieper for her carful technical assistance. We are also grateful to ProfessorR. Hess and Dr.J. Gelzer (Ciba-Geigy, Basel) for the supply of rifampicin.     

Some new data concerning effect of actinomycin D on early chick embryos

Zusammenfassung Actinomycin D führte beim Hühnerembryo zu einer deutlichen Hemmung der Herzentwicklung nach Inkubation im Nährmedium während der Entwicklungsstadien 3 und 3⁺. Nach Vorbehandlung der Stadien 3–7 und anschliessender Kultur in actinomycin D-freiem Medium fanden sich Fehlbildungen von Herz, ZNS und Somiten, die in ihrer Häufigkeit von den betroffenen Entwicklungsphasen abhängig sind.

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This study was supported by a grant from the Rutgers University Research Council No. 07-2189.     

On the synthesis of poliovirus RNA at supraoptimal temperatures

Riassunto La scarsa incorporazione di precursori dello ARN in cellule infette da poliovirus ed incubate a 41,5°C è dovuta ad una inibizione della sintesi dello ARN virale più che non ad una sua digestione ad opera di nucleasi.

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Work supported by a Grant of Consiglio Nazionale delle Ricerche, Rome.     

A star in a 15.2-year orbit around the supermassive black hole at the centre of the Milky Way

Many galaxies are thought to have supermassive black holes at their centres-more than a million times the mass of the Sun. Measurements of stellar velocities and the discovery of variable X-ray emission have provided strong evidence in favour of such a black hole at the centre of the Milky Way, but have hitherto been unable to rule out conclusively the presence of alternative concentrations of mass. Here we report ten years of high-resolution astrometric imaging that allows us to trace two-thirds of the orbit of the star currently closest to the compact radio source (and massive black-hole candidate) Sagittarius A*. The observations, which include both pericentre and apocentre passages, show that the star is on a bound, highly elliptical keplerian orbit around Sgr A*, with an orbital period of 15.2 years and a pericentre distance of only 17 light hours. The orbit with the best fit to the observations requires a central point mass of (3.7 +/- 1.5) x 10(6) solar masses (M(*)). The data no longer allow for a central mass composed of a dense cluster of dark stellar objects or a ball of massive, degenerate fermions.