"My bones shall rise again" : war veterans, spirits and land reform in Zimbabwe

Zimbabawe's land reform programme has attracted the attention of many commentators and has elicited a multiplicity of interpretations. By and large, however, this exercise has been politicized, that is, those who have criticized or justified the programme have done so on political or economic grounds. The relationship between land and indigenous religion has not been sufficiently examined. The present paper explores this relationship through an analysis of the reburial of fallen heroes, spearheaded by Zimbabwean war veterans. It argues that the reburial activities reflect Zimbabwe's incorporation of religion into political discourse and that the Shona people understand this link in terms of their traditional cosmology. As ritual practice, reburials are effective tools for shaping the politics of restitution, nationbuilding and moral accountability. [Book abstract

Low energy effective action on a self-gravitating D-brane

Recently the study of braneworld on the self-gravitating D-brane has been initiated and derived the gravitational equation on the brane by holographic and geometrical projection methods. Surprisingly, in common with these two methods, the matter on the brane cannot be the source of the gravity on the brane at leading order. In this paper we will propose the low energy effective action on the D-brane coupled with gravity which derives the same results.Comment: 8 pages, minor corrections, accepted for publication in Physical Review

Observation of the Halo of NGC 3077 Near the "Garland" Region Using the Hubble Space Telescope

We report the detection of upper main sequence stars and red giant branch stars in the halo of an amorphous galaxy, NGC3077. The observations were made using Wide Field Planetary Camera~2 on board the Hubble Space Telescope. The red giant branch luminosity function in I-band shows a sudden discontinuity at I = 24.0 +- 0.1 mag. Identifying this with the tip of the red giant branch (TRGB), and adopting the calibration provided by Lee, Freedman, & Madore (1993) and the foreground extinction of A_B = 0.21 mag, we obtain a distance modulus of (m-M)_0 = 27.93 +- 0.14(random) +- 0.16(sys). This value agrees well with the distance estimates of four other galaxies in the M81 Group. In addition to the RGB stars, we observe a concentration of upper main sequence stars in the halo of NGC3077, which coincides partially with a feature known as the ``Garland''. Using Padua isochrones, these stars are estimated to be <150 Myrs old. Assuming that the nearest encounter between NGC3077 and M81 occurred 280 Myrs ago as predicted by the numerical simulations (Yun 1997), the observed upper main sequence stars are likely the results of the star formation triggered by the M81-NGC3077 tidal interaction.Comment: 15 pages, 8 figures. Accepted for publication in Astrophysical Journa

Morphological and molecular characterisation of Streptomyces spp. which suppress pathogenic fungi

Streptomyces species are aerobes and chemoorganotrophic bacteria. These microorganisms produce a wide range of industrially significant compounds, specifically antibiotics and anti fungal substances. The objective of this study was to characterise soil-borne Streptomyces isolates using morphological and molecular traits in order to identify them to species level, and leverage from their potential to suppress the growth of Aspergillus flavus , Fusarium oxysporum and Penicillium italicum . Twenty-seven soil-borne putative Streptomyces, which elicited comprehensive\ua0antimicrobial activity against Aspergillus flavus, Fusarium oxysporum and Penicillium italicum, in a previous study, were evaluated. On the basis of morphology, the bacteria resembled the genus Streptomyces. Initially, colonies phenotypically appeared to have a relatively smooth surface but as growth progressed the bacteria developed a weft of aerial mycelium granular, powdery or velvety in appearance. Bacteria produced a wide variety of pigments which in turn were responsible for the colour of the vegetative and aerial mycelia, colour ranged from white to cream or buff shades and yellow to orange or brown. Microscopic analyses and morphological characteristics generated sub-groups of the isolates and clustered them according to their similarities. One bacterial strain was randomly selected from each cluster and investigated using molecular characteristics. Partial 16S rDNAs from the selected representative isolates from each subgroup, were sequenced and phylogenetic analysis performed. The 16S\ua0rDNA\ua0sequences of the isolates indicated that they were related to\ua0 Streptomyces species: S. bungoensis , S. thermocarboxydus , S. corchorusii and S. lasaliensis, that are known secondary metabolite producers possessing antimicrobial activity against plant pathogens.Les esp\ue8ces de Streptomyces sont des bact\ue9ries a\ue9robies et chimio-organotrophes. Ces micro-organismes produisent une large gamme de compos\ue9s d\u2019importance industrielle, en particulier des antibiotiques et des substances antifongiques. L\u2019objectif de cette \ue9tude \ue9tait de caract\ue9riser les isolats de Streptomyces transmis par le sol \ue0 l\u2019aide de traits morphologiques et mol\ue9culaires afin de les identifier au niveau de l\u2019esp\ue8ce, et de tirer parti de leur potentiel \ue0 supprimer la croissance d\u2019 Aspergillus flavus , Fusarium oxysporum et Penicillium italicum . Vingt-sept Streptomyces putatifs transmis par le sol, qui ont suscit\ue9 une activit\ue9 antimicrobienne compl\ue8te contre Aspergillus flavus, Fusarium oxysporum et Penicillium italicum, dans une \ue9tude pr\ue9c\ue9dente, ont \ue9t\ue9 \ue9valu\ue9s. Sur la base de la morphologie, les bact\ue9ries ressemblaient au genre Streptomyces. Au d\ue9part, les colonies semblaient ph\ue9notypiquement avoir une surface relativement lisse, mais au fur et \ue0 mesure que la croissance progressait, les bact\ue9ries d\ue9veloppaient une trame de myc\ue9lium a\ue9rien d\u2019aspect granuleux, poudreux ou velout\ue9. Les bact\ue9ries produisaient une grande vari\ue9t\ue9 de pigments qui \ue0 leur tour \ue9taient responsables de la couleur des myc\ue9liums v\ue9g\ue9tatifs et a\ue9riens, la couleur variait du blanc au cr\ue8me ou au chamois et du jaune \ue0 l\u2019orange ou au brun. Des analyses microscopiques et des caract\ue9ristiques morphologiques ont g\ue9n\ue9r\ue9 des sous-groupes d\u2019isolats et les ont regroup\ue9s en fonction de leurs similitudes. Une souche bact\ue9rienne a \ue9t\ue9 s\ue9lectionn\ue9e au hasard dans chaque groupe et \ue9tudi\ue9e en utilisant des caract\ue9ristiques mol\ue9culaires. Des ADNr 16S partiels provenant des isolats repr\ue9sentatifs s\ue9lectionn\ue9s de chaque sous-groupe ont \ue9t\ue9 s\ue9quenc\ue9s et une analyse phylog\ue9n\ue9tique a \ue9t\ue9 effectu\ue9e. Les s\ue9quences d\u2019ADNr 16S des isolats ont indiqu\ue9 qu\u2019ils \ue9taient apparent\ue9s aux esp\ue8ces de Streptomyces: S. bungoensis , S. thermocarboxydus , S. corchorusii et S. lasaliensis, qui sont des producteurs de m\ue9tabolites secondaires connus poss\ue9dant une activit\ue9 antimicrobienne contre les phytopathog\ue8nes

In vitro suppression of pathogenic fungi by Streptomyces spp.

The use of living organisms or natural enemies of pathogens to control their populations is called biological disease control. It involves harnessing and introduction of exotic species of microorganism in a natural form, with the intention of controlling pathogens that may exist naturally in the same ecosystem. Prospects for biological control of Aspergillus flavus , Fusarium oxysporum and Penicillium italicum were investigated using Streptomyces spp. isolated from Chinhoyi University of Technology Farm soils in Mashonaland West, Zimbabwe. Twenty seven Streptomyces spp were obtained from the soil, and screened for antimicrobial activity and antagonism in in vitro pathogen inhibition assays, replicated thrice. Although majority of the isolates tested elicited no effect on test pathogens, 22% of the Streptomyces isolates were able to effectively suppress A. flavus, F. oxysporum and P. italicum by at least 55%. There was a significant interaction between Streptomyces isolates and pathogen (A. flavus, F. oxysporum and P. italicum) (P&lt;0.05) on fungal radial growth at days 7, 10 and 14 after pathogen-Streptomyces incubation. Antimicrobial potential against individual and multiple test pathogens was observed, with CUT-Streptomyces 4, CUT-Streptomyces 10, CUT-Streptomyces 11, CUT-Streptomyces 20 and CUT-Streptomyces 23 showing the greatest antimicrobial activity. CUT-Streptomyces isolates have the potential to suppress A. flavus, F. oxysporum and P. italicum in vitro.L\u2019utilisation d\u2019organismes vivants ou d\u2019ennemis naturels d\u2019agents pathog\ue8nes pour contr\uf4ler leurs populations est appel\ue9e contr\uf4le biologique des maladies. Il s\u2019agit d\u2019exploiter et d\u2019introduire des esp\ue8ces exotiques de microorganismes sous une forme naturelle, dans le but de contr\uf4ler les agents pathog\ue8nes pouvant exister naturellement dans le m\ueame \ue9cosyst\ue8me. Les perspectives de lutte biologique contre Aspergillus flavus , Fusarium oxysporum et Penicillium italicum ont \ue9t\ue9 \ue9tudi\ue9es \ue0 l\u2019aide de Streptomyces spp. isol\ue9es des sols agricoles de l\u2019Universit\ue9 de Technologie de Chinhoyi \ue0 Mashonaland West, Zimbabwe. Vingt-sept Streptomyces spp ont \ue9t\ue9 obtenus du sol et cribl\ue9s pour l\u2019activit\ue9 antimicrobienne et l\u2019antagonisme dans des tests d\u2019inhibition des agents pathog\ue8nes in vitro, r\ue9pliqu\ue9s trois fois. Bien que la majorit\ue9 des isolats test\ue9s ne provoquent aucun effet sur les agents pathog\ue8nes test\ue9s, 22% des isolats de Streptomyces sont capables de supprimer efficacement au moins 55% des A. flavus, F. oxysporum et P. italicum. Il y avait une interaction significative entre les isolats de Streptomyces et l\u2019agent pathog\ue8ne (A. flavus, F. oxysporum et P. italicum) (P&lt; 0.05) lors de la croissance radiale des champignons aux 7\ue8me, 10\ue8me et 14\ue8me jours apr\ue8s l\u2019incubation de l\u2019agent pathog\ue8ne-Streptomyces. Un potentiel antimicrobien contre des agents pathog\ue8nes individuels et multiples a \ue9t\ue9 observ\ue9. CUT-Streptomyces 4, CUT-Streptomyces 10, CUT-Streptomyces 11, CUT-Streptomyces 20 et CUT-Streptomyces 23 ont montr\ue9 l\u2019activit\ue9 antimicrobienne la plus \ue9lev\ue9e. Les isolats de CUT-Streptomyces ont le potentiel de supprimer A. flavus, F. oxysporum et P. italicum in vitro

The Tip of the Red Giant Branch Distance to the Large Magellanic Cloud

We present the I-band luminosity function of the red giant branch stars in the Large Magellanic Cloud (LMC) using the data from the Magellanic Clouds Photometric Survey (Zaritsky, Harris & Thompson, 1997). Selecting stars in uncrowded, low-extinction regions, a discontinuity in the luminosity function is observed at I_0 = 14.54 mag. Identifying this feature with the tip of the red giant branch (TRGB), and adopting an absolute TRGB magnitude of -4.05 +- 0.04 mag based on the calibration of Lee, Freedman & Madore (1993), we obtain a distance modulus of 18.59 +- 0.09 (random) +- 0.16 (systematic) mag. If the theoretical TRGB calibration provided by Cassisi & Salaris (1997) is adopted instead, the derived distance would be 4% greater. The LMC distance modulus reported here, 18.59 +- 0.09, is larger by 0.09 mag (1-sigma) than the value that is most commonly used in the extragalactic distance scale calibrated by the period-luminosity relation of the Cepheid variable stars. Our TRGB distance modulus agrees with several RR Lyrae distances to the LMC based on HIPPARCOS parallaxes. Finally, we note that using the same MCPS data, we obtain a distance modulus of 18.29 +- 0.03 mag using the red clump method, which is shorter by 0.3 mag compared to the TRGB estimate.Comment: 19 pages, 5 figure

Volatile constituents of fruit pulp of Strychnos cocculoides (Baker) growing in Malawi using solid phase microextraction

Volatile constituents of the edible pulp of Strychnos cocculoides (Monkey orange) were extracted using solid phase microextraction (SPME) and their identity established by GC–FID and GC–MS systems. Six compounds were extracted and identified: isobutyl acetate, 53.2%; 2-methylbutyl acetate, 12.8%; ethyl-2-methylbutyrate, 10.5%; 2, 6-ditetrabutyl-4-methyl-phenol, 8.4%; butyl-2-methyl butyrate, 6.7% and geranyl acetate, 3.1%. These accounted for 94.7% of the volatile constituents in the pulp. Thus, the acetate and butyrate esters were the most abundant volatiles in the edible pulp of the ripe fruit.Carnegie Regional Initiative in Science Education (Carnegie-RISE) through the Southern Africa Biochemistry and Informatics for Natural Products (SABINA) network and the ACP EU through the POL-SABINA network. Open Access funded by SAAB.http://www.elsevier.com/locate/sajbhb2016Biochemistr

The enigmatic pair of dwarf galaxies Leo IV and Leo V: coincidence or common origin?

We have obtained deep photometry in two 1x1 degree fields covering the close pair of dwarf spheroidal galaxies (dSph) Leo IV and Leo V and part of the area in between. We find that both systems are significantly larger than indicated by previous measurements based on shallower data and also significantly elongated. With half-light radii of r_h=4'.6 +- 0'.8 (206 +- 36 pc) and r_h=2'.6 +- 0'.6 (133 +- 31 pc), respectively, they are now well within the physical size bracket of typical Milky Way dSph satellites. Their ellipticities of epsilon ~0.5 are shared by many faint (M_V>-8) Milky Way dSphs. The large spatial extent of our survey allows us to search for extra-tidal features with unprecedented sensitivity. The spatial distribution of candidate red giant branch and horizontal branch stars is found to be non-uniform at the ~3 sigma level. This substructure is aligned along the direction connecting the two systems, indicative of a possible `bridge' of extra-tidal material. Fitting the stellar distribution with a linear Gaussian model yields a significance of 4 sigma for this overdensity, a most likely FWHM of ~16 arcmin and a central surface brightness of ~32 mag arcsec^{-2}. We investigate different scenarios to explain the close proximity of Leo IV and Leo V and the possible tidal bridge between them. Orbit calculations demonstrate that they are unlikely to be remnants of a single disrupted progenitor, while a comparison with cosmological simulations shows that a chance collision between unrelated subhalos is negligibly small. Leo IV and Leo V could, however, be a bound `tumbling pair' if their combined mass exceeds 8 +- 4 x 10^9 M_sun. The scenario of an internally interacting pair appears to be the most viable explanation for this close celestial companionship. (abridged)Comment: 9 pages, 8 figures, small number of minor textual changes, accepted for publication in Astrophysical Journa

The Hubble Space Telescope Key Project on the Extragalactic Distance Scale XXIV: The Calibration of Tully-Fisher Relations and the Value of the Hubble Constant

This paper presents the calibration of BVRIH$ Tully-Fisher relations based on Cepheid distances to 21 galaxies within 25 Mpc, and 23 clusters within 10,000 km/s. These relations have been applied to several distant cluster surveys in order to derive a value for the Hubble constant, H0, mainly concentrating on an I-band all-sky survey by Giovanelli and collaborators which consisted of total I magnitudes and 50% linewidth data for ~550 galaxies in 16 clusters. For comparison, we also derive the values of H0 using surveys in B-band and V-band by Bothun and collaborators, and in H-band by Aaronson and collaborators. Careful comparisons with various other databases from literature suggest that the H-band data, whose magnitudes are isophotal magnitudes extrapolated from aperture magnitudes rather than total magnitudes, are subject to systematic uncertainties. Taking a weighted average of the estimates of Hubble constants from four surveys, we obtain H0 = 71 +- 4 (random) +- 7 (systematic) km/s/Mpc. We have also investigated how various systematic uncertainties affect the value of H0 such as the internal extinction correction method used, Tully-Fisher slopes and shapes, a possible metallicity dependence of the Cepheid period-luminosity relation and cluster population incompleteness bias.Comment: 34 pages, 13 figure

Peripheral Blood CD64 Levels Decrease in Crohn's Disease following Granulocyte and Monocyte Adsorptive Apheresis

Granulocyte and monocyte adsorptive apheresis (GMA) is reportedly useful as induction therapy for Crohn's disease (CD). However, the effects of GMA on CD64 have not been well characterized. We report here our assessment of CD64 expression on neutrophils before and after treatment with GMA in two patients with CD. The severity of CD was assessed with the CD activity index (CDAI). The duration of each GMA session was 60 min at a flow rate of 30 ml/min as per protocol. CD64 expression on neutrophils was measured by analyzing whole blood with a FACScan flow cytometer. In case 1, CD64 levels after each session of GMA tended to decrease compared to pretreatment levels, whereas in case 2, CD64 levels dropped significantly after treatment. The CDAI decreased after GMA in both cases 1 and 2. A significant correlation was noted between CDAI scores and CD64 levels in both cases. In conclusion, GMA reduced blood CD64 levels, which would be an important factor for the decrease of CDAI scores