Purification of all thirteen polypeptides of bovine heart cytochrome c oxidase from one aliquot of enzyme Characterization of bovine fetal heart cytochrome c oxidase

AbstractA protocol has been worked out for separating all thirteen different polypeptides in the beef heart cytochrome c oxidase complex from a single aliquot of enzyme. This involves an initial separation of polypeptides by gel filtration on a Biogel P-60 column in SDS, a step which purifies subunits CIV and CVIII and gives mixtures of CV+CVI, ASA, AED and STA, as well as CVII, CIX and IHQ. These mixtures are then resolved by reverse-phase high-performance liquid chromatography. The separation procedures have been applied to fetal heart cytochrome c oxidase of gestation between 100 and 200 days. No differences were found in the N-terminal sequences of any of the cytoplasmically made subunits or in the entire sequence of CIX between late fetal and adult forms of the enzyme

Dust-penetrated morphology in the high-redshift universe: clues from NGC 922

Results from the Hubble Deep Field (HDF) North and South show a large percentage of high-redshift galaxies whose appearance falls outside traditional classification systems. The nature of these objects is poorly understood, but sub-mm observations indicate that at least some of these systems are heavily obscured (Sanders 2000). This raises the intriguing possibility that a physically meaningful classification system for high-redshift galaxies might be more easily devised at rest-frame infrared wavelengths, rather than in the optical regime. Practical realization of this idea will become possible with the advent of the Next Generation Space Telescope (NGST). In order to explore the capability of NGST for undertaking such science, we present NASA-IRTF and SCUBA observations of NGC 922, a chaotic system in our local Universe which bears a striking resemblance to objects such as HDF 2-86 (z=0.749) in the HDF North. If objects such as NGC 922 are common at high-redshifts, then this galaxy may serve as a local morphological `Rosetta stone' bridging low and high-redshift populations. In this paper we demonstrate that quantitative measures of galactic structure are recoverable in the rest-frame infrared for NGC 922 seen at high redshifts using NGST, by simulating the appearance of this galaxy at redshifts z=0.7 and z=1.2 in rest-frame K'. Our results suggest that the capability of efficiently exploring the rest-wavelength IR morphology of high-z galaxies should probably be a key factor in deciding the final choice of instruments for the NGST.Comment: 7 pages, 12 Figures. Accepted for publication in A&A. Better version of the figures can be found at http://www.inaoep.mx/~puerari/ngs

The ACS Virgo Cluster Survey XV. The Formation Efficiencies of Globular Clusters in Early-Type Galaxies: The Effects of Mass and Environment

The fraction of stellar mass contained in globular clusters (GCs), also measured by number as the specific frequency, is a fundamental quantity that reflects both a galaxy's early star formation and its entire merging history. We present specific frequencies, luminosities, and mass fractions for the globular cluster systems of 100 early-type galaxies in the ACS Virgo Cluster Survey, the largest homogeneous catalog of its kind. We find that 1) GC mass fractions can be high in both giants and dwarfs, but are universally low in galaxies with intermediate luminosities. 2) The behavior of specific frequency across galaxy mass is dominated by the blue GCs. 3) The GC fractions of low-mass galaxies exhibit a dependence on environment. Nearly all dwarf galaxies with high GC fractions are within 1 Mpc of the cD galaxy M87, presenting the first strong evidence that GC formation in dwarfs is biased toward dense environments. 4) GC formation in central dwarfs is biased because their stars form earliest and most intensely. Comparisons to the Millennium Simulation show that central dwarfs have older stellar populations and form more stars at higher star formation rates (SFRs) and SFR surface densities. The SFR surface density in simulated dwarfs peaks before the total SFR, naturally producing GC populations that are older and more metal-poor than the field stars. 5) Dwarfs within ~40 kpc of the giant ellipticals M87 and M49 are red and have few or no GCs, suggesting that they have been tidally stripped and have contributed their GCs to the halos of their giant neighbors. The central dwarfs with high GC mass fractions are thus likely to be the survivors most similar to the protogalaxies that assembled the rich M87 globular cluster system.(Abridged)Comment: 27 pages, 21 figures, 7 tables. Accepted for publication in the Astrophysical Journa

Demography, trade and state power: a tripartite model of medieval farming/language dispersals in the Ryukyu Islands

Hunter-gatherer occupations of small islands are rare in world prehistory and it is widely accepted that island settlement is facilitated by agriculture. The Ryukyu Islands contradict that understanding on two counts: not only did they have a long history of hunter-gatherer settlement, they also have a very late date for the onset of agriculture, which only reached the archipelago between the 8th and 13th centuries AD. Here, we combine archaeology and linguistics to propose a tripartite model for the spread of agriculture and Ryukyuan languages to the Ryukyu Islands. Employing demographic growth, trade/piracy and the political influence of neighbouring states, this model provides a synthetic yet flexible understanding of farming/language dispersals in the Ryukyus within the complex historical background of medieval East Asia.Introduction Methods Results - Archaeological Approach -- Demographic growth -- Trade/piracy -- State intervention - Linguistic Approach -- Linguistic inferences about the most probable tree structure -- Linguistic inferences about the most probable homeland of Proto-Ryukyuan -- Linguistic inferences about the most probable break-up time of Proto-Kyushu-Ryukyuan -- Inferences about the most probable linguistic outcome of the migration Discussion Conclusion

Análise do efeito de nanopartículas de prata contra células aderidas e biofilmes de Candida albicans e Candida glabrata

O aumento na resistência dos biofilmes de Candida à terapia antifúngica convencional tem despertado o interesse no uso da prata como um agente antimicrobiano. Assim, o objetivo deste trabalho foi avaliar a eficácia antifúngica de nanopartículas de prata (NPs) contra células aderidas e biofilmes de Candida albicans e Candida glabrata. Métodos: NPs esféricas (5 nm) foram sintetizadas através da redução do nitrato de prata pelo citrato de sódio. Testes de mínima concentração inibitória (MCI) foram realizados para as duas espécies de Candida de acordo com o método da microdiluição. NPs foram aplicadas sobre células aderidas (2 hrs) e biofilmes (48 hrs), e após 24 horas de contato os biofilmes resultantes foram caracterizados através da contagem do número de unidades formadoras de colônias (UFCs) e quantificação da biomassa total. Resultados: Os valores de MCI para C. glabrata foram maiores (0,4 – 3,3 µg/mL) do que para C. albicans (0,4 – 1,6 µg/mL). NPs foram mais efetivas na redução da biomassa total quando aplicadas sobre células aderidas do que sobre biofilmes pré-formados. NPs também foram altamente efetivas na redução das UFCs quando aplicadas sobre as células aderidas de C. glabrata (~70%) e respectivos biofilmes (~50%). Para as cepas de C. albicans o efeito não foi tão notório, mas também existiu uma redução no número de UFCs. Conclusão: NPs apresentam potencial como agente antifúngico alternativo no controle de infecções por espécies de Candida