Rapid growth of black holes in massive star-forming galaxies

The tight relationship between the masses of black holes and galaxy spheroids in nearby galaxies implies a causal connection between the growth of these two components. Optically luminous quasars host the most prodigious accreting black holes in the Universe, and can account for greater than or approximately equal to 30 per cent of the total cosmological black-hole growth. As typical quasars are not, however, undergoing intense star formation and already host massive black holes (> 10(8)M(o), where M(o) is the solar mass), there must have been an earlier pre-quasar phase when these black holes grew (mass range approximately (10(6)-10(8))M(o)). The likely signature of this earlier stage is simultaneous black-hole growth and star formation in distant (redshift z > 1; >8 billion light years away) luminous galaxies. Here we report ultra-deep X-ray observations of distant star-forming galaxies that are bright at submillimetre wavelengths. We find that the black holes in these galaxies are growing almost continuously throughout periods of intense star formation. This activity appears to be more tightly associated with these galaxies than any other coeval galaxy populations. We show that the black-hole growth from these galaxies is consistent with that expected for the pre-quasar phase.     

Observations on the developmental biology of Cicindela arenicola Rumpp (Coleoptera: Cicindelidae)

Cicindela arenicola Rumpp is being considered for threatened and endangered status by the U.S. Fish and Wildlife Service. Little is known about the developmental biology of this species. Adults of C. arenicola were active from April through late June and late August through early November, but generally they were not on the surface when temperatures were below 19 C or above 45 C, or when conditions were windy, cloudy, or rainy. Mating and egg-laying occurred only during the spring. Five size classes (1-,2-,3-,4-, and 5-mm diameters) of larval burrow openings were observed. Burrows of 5 mm had a mean depth of 42.23 ± 8.81 cm (1 S.D.). Larvae of C. arenicola were active from April through June and late September through mid-November. Developmental times and larval size were affected by food supplementation. Nearly all food-supplemented, 1-mm, first instars molted to larger second instars of3-mm diameter. Most nonsupplemented larvae spent several months as 2-mm second instars before growing to 3 mm in diameter. Food-supplemented larvae reached the third instar in approximately 13 months, while nonsupplemented larvae took slightly over two years to reach this stage. Development from egg to adult was estimated at two years for food-supplemented larvae and three and one-half to four years for nonsupplemented larvae. Cattle had a significant effect on larval mortality. A high percentage (76-80%) of larval C. arenicola that were stepped on by cattle never reopened their burrows. Only 14% of undisturbed larvae never reopened their burrows. Approximately 15% of 150 larvae marked in 1988 reopened burrows in 1989.     

Visualizing heavy fermions emerging in a quantum critical Kondo lattice

In solids containing elements with f orbitals, the interaction between f-electron spins and those of itinerant electrons leads to the development of low-energy fermionic excitations with a heavy effective mass. These excitations are fundamental to the appearance of unconventional superconductivity and non-Fermi-liquid behaviour observed in actinide- and lanthanide-based compounds. Here we use spectroscopic mapping with the scanning tunnelling microscope to detect the emergence of heavy excitations with lowering of temperature in a prototypical family of cerium-based heavy-fermion compounds. We demonstrate the sensitivity of the tunnelling process to the composite nature of these heavy quasiparticles, which arises from quantum entanglement of itinerant conduction and f electrons. Scattering and interference of the composite quasiparticles is used to resolve their energy-momentum structure and to extract their mass enhancement, which develops with decreasing temperature. The lifetime of the emergent heavy quasiparticles reveals signatures of enhanced scattering and their spectral lineshape shows evidence of energy-temperature scaling. These findings demonstrate that proximity to a quantum critical point results in critical damping of the emergent heavy excitation of our Kondo lattice system.     

A single origin of phenylketonuria in Yemenite Jews

Phenylketonuria (PKU) is a metabolic disease caused by recessive mutations of the gene encoding the hepatic enzyme phenylalanine hydroxylase (PAH). The incidence of PKU varies widely across different geographic areas, and is highest (about 1 in 5,000 live births) in Ireland and western Scotland, and among Yemenite Jews. A limited number of point mutations account for most of the PKU cases in the European population. Here we report that a single molecular defect--a deletion spanning the third exon of the PAH gene--is responsible for all the PKU cases among the Yemenite Jews. Examination of a random sample of Yemenite Jews using a molecular probe that detects the carriers of this deletion indicated a high frequency of the defective gene in this community. Although the deleted PAH gene was traced to 25 different locations throughout Yemen, family histories and official documents of the Yemenite Jewish community showed that the common ancestor of all the carriers of this genetic defect lived in San'a, the capital of Yemen, before the eighteenth century.     

Inhibitory effect of beta-ecdysone on protein synthesis by blowfly fat body in vitro

Synthesis of blow fly calliphorin and other blood proteins by larval fat body in organ culture is inhibited by beta-ecdysone. The findings suggest a novel function for the hormone.     

Use of the exo-β-(1→3) glucanase from basidiomycete QM 806 in studies on yeast

Résumé L'exo--(13) glucanasem isolée duBasidiomycete QM 806 a été utilisée avec succès pour l'analyse des polysaccharides de la paroi cellulaire de la levureSaccharomyces cerevisiae et pour la formation de protoplastes à partir deSaccharomyces cerevisiae etWickerhamia fluorescens.

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Acknowledgments. We are indepted to MissE. Sigarlakie and MissE. Wespi for technical assistance during the course of this investigation.