Alkaloids ofBerberis laurina Billb. II. Two new phenolic biscoclaurine alkaloids

Zusammenfassung Die Isolierung von zwei neuen dauricinartigen AlkaloÏden, Espinin and Espinidin, ausBerberis laurina, und deren Strukturaufklärung durch Spektroskopie und Degradation werden beschrieben.     

The sterols of two hadromerida sponges

Summary Sterols were extracted and identified from 2 marine sponges,Aaptos aaptos andSuberites domuncula. The sponges contained conventional C₂₆–C₃₀ sterols with a saturated ring system. Minor amounts of cholest-7-en-3-ol and cholesterol were also present. Cholestanol and 24-ethylcholestanol were the major components of the sterol mixtures.We thank Prof. L. Boniforti (Istituto Superiore di Sanità, Roma) for CG-MS analysis, Prof. R. Pronzato (Istituto di Zoologia dell'Università di Genova) for identifying the sponges and A. Senatore for G.C. measurements. This research was supported by grants of Ministero P.I. and C.N.R.     

Gorenstein平坦预包络和预解式

我们在［７］中引进了Ｇｏｒｅｎｓｔｅｉｎ平坦模。本文将这类模的刻画推广到任意ｎ－Ｇｏｒｅｎｓｔｅｉｎ环上，并利用这类模刻画了ｎ－Ｇｏｒｅｓｔｅｉｎ环。而且，我们证明了任意ｎ－Ｇｏｒｅｎｓｔｅｉｎ环上Ｇｏｒｅｎｓｔｅｉｎ平坦预包络的存在性，并证得得这种环关于Ｇｏｒｅｎｓｔｅｉｎ平坦模的内射类的整体维数至多为ｎ－２，当ｎ≤１时，该整体维数为零。     

An infrared flash contemporaneous with the gamma-rays of GRB 041219a

The explosion that results in a cosmic gamma-ray burst (GRB) is thought to produce emission from two physical processes: the central engine gives rise to the high-energy emission of the burst through internal shocking, and the subsequent interaction of the flow with the external environment produces long-wavelength afterglows. Although observations of afterglows continue to refine our understanding of GRB progenitors and relativistic shocks, gamma-ray observations alone have not yielded a clear picture of the origin of the prompt emission nor details of the central engine. Only one concurrent visible-light transient has been found and it was associated with emission from an external shock. Here we report the discovery of infrared emission contemporaneous with a GRB, beginning 7.2 minutes after the onset of GRB 041219a (ref. 8). We acquired 21 images during the active phase of the burst, yielding early multi-colour observations. Our analysis of the initial infrared pulse suggests an origin consistent with internal shocks.