Testicular myxosporidiasis in anurans, with a description of Myxobolus fallax n. sp.

During studies of amphibian sperm cryopreservation, a new species of myxosporidean parasite (Myxozoa, Myxosporae) was observed in the testes of the Australian dwarf green tree frog Litoria fallax (Peters). Myxosporidiasis was found to have no affect on L. fallax body condition or sperm numbers. Myxobolus spores from L. fallax are morphologically distinct from Myxobolus hylae spores (infecting the sympatric Litoria aurea Lesson) and the three previously named (exotic to Australia) Myxobolus species found in anurans. Myxobolus fallax n. sp. is characterised by: pseudocyst white, spherical to ovoid, 141 x74 to 438 x337 mum in diameter (mature); plasmodium with spores loosely arranged within interior. Spores ovoid 13.4 +/- 0.5 (12.6-14.6) mum length, 9.5 +/- 0.4 (8.3-10.6) mum width, 6.8 +/- 0.4 (6.5-7.6) mum depth, 1.4 +/- 0.1 (1.3-1.6) length/width; polar capsules broadly pyriform and equal in size 4.2 +/- 0.3 (3.3-4.7) mum length, 2.4 +/- 0.2 (2.1-2.8) mum width; filament coils 7-8, wound tightly and perpendicular to the longitudinal axis of the capsule; polar filament 34 +/- 7.0 (18-50) mum length; intercapsular appendix and sutural ridge folds absent; and iodinophilous vacuole and mucous envelope lacking. In addition to this new species, data from archival samples of M. hylae are provided which show two morphologically distinct spore types. Both appeared rarely in the same pseudocysts and we cautiously retain the single species.

Combining the analyses of introgressive hybridisation and linkage mapping to investigate the genetic architecture of population divergence in the lake whitefish (Coregonus clupeaformis, Mitchill)

Adaptation and reproductive isolation, the engines of biological diversity, are still elusive when discussing the genetic bases of speciation. Namely, the number of genes and magnitude of selection acting positively or negatively on genomic traits implicated in speciation is contentious. Here, we describe the first steps of an ongoing research program aimed at understanding the genetic bases of population divergence and reproductive isolation in the lake whitefish (Coregonus clupeaformis). A preliminary linkage map originating from a hybrid cross between dwarf and normal ecotypes is presented, whereby some of the segregating AFLP markers were found to be conserved among natural populations. Maximum-likelihood was used to estimate hybrid indices from non-diagnostic markers at 998 AFLP loci. This allowed identification of the most likely candidate loci that have been under the influence of selection during the natural hybridisation of whitefish originating from different glacial races. As some of these loci could be identified on the linkage map, the possibility that selection of traits in natural populations may eventually be correlated to specific chromosomal regions was demonstrated. The future prospects and potential of these approaches to elucidate the genetic bases of adaptation and reproductive isolation among sympatric ecotypes of lake whitefish is discussed.

MOND virial theorem applied to a galaxy cluster

Large values for the mass-to-light ratio (ϒ) in self-gravitating systems is one of the most important evidences of dark matter. We propose a expression for the mass-to-light ratio in spherical systems using MOND. Results for the COMA cluster reveal that a modification of the gravity, as proposed by MOND, can reduce significantly this value.

Phytomass production and nutrient accumulation by green manure species

Green manuring is recognized as a viable alternative to improve nutrient cycling in soils. The aim of this study was to evaluate the phytomass production and nutrient accumulation in shoots of the summer green manures jack bean [Canavalia ensiformis (L.) DC.], dwarf pigeon pea (Cajanus cajanvar var. Flavus DC.), dwarf mucuna [Mucuna deeringiana (Bort) Merr] and sunn hemp (Crotalaria juncea L.), under nitrogen fertilization and/or inoculation with N-fixing bacteria. A split plot design was arranged with the four Fabaceae species as main plots and nitrogen fertilization (with and without) and inoculation with diazotrophic bacteria (with and without) as the subplots, in a 2² factorial. The experiment was arranged as a randomized complete block design with four replications. In the conditions of this trial, the sunn hemp had the highest production of shoot phytomass (12.4 Mg ha-1) and nutrient accumulation, while the dwarf mucuna had the lowest production of shoot phytomass (3.9 Mg ha-1) and nutrient accumulation. The results showed no effect of nitrogen fertilization or inoculation with N-fixing bacteria on the production of shoot phytomass and nutrient accumulation, except for inoculation without nitrogen fertilization, resulting in greater P accumulation (p <0.05) in the sunn hemp and greater Zn and Mn accumulation in the dwarf mucuna. These findings indicate that N fertilization or inoculation with N2-fixing bacteria for Fabaceae are low efficiency practices in the edaphoclimatic conditions of this study.

Estudio de las afecciones causadas por el virus MRDV, agente del Mal de Río Cuarto, en plantas de gramínea

El Mal de Río Cuarto es una enfermedad virósica causada por el Maize Rorgh Dwarf Virus (MRDV), el cual es transmitido por el insecto vector Delphacodes kuscheli. Esta enfermedad provoca cuantiosas pérdidas económicas sobre todo en maíz, afectando la producción de granos y forraje. El presente proyecto, empleando plantas de maíz cuya infección será provocada y plantas de sorgo y avena con síntomas visibles de la enfermedad, recolectadas a campo, se propone a lo largo de tres años: realizar un estudio anatómico, comparativo entre variedades susceptibles y ligeramente resistentes de maíz para determinar en qué etapa fenológica de la planta se observan las primeras anomalías; localizar partículas virales y estudiar los cambios celulares en orgánulos y pared celular por microscopía electrónica de transmisión y analizar la relación de auxina (IAA) endógena/IAA-oxidasa en enaciones de diferentes estadíos de su desarrollo, a fin de establecer correlaciones hormonales y enzimáticas con la proliferación de tejidos vasculares observada en estas agallas foliares. El conocimiento de las interrelaciones huésped-patógeno, en este caso particular gramínea-virus, brindará la posibilidad de obtener un modelo que en el futuro pueda servir de base a la Biología Molecular a fin de incorporar caracteres de resistencia a enfermedades en cultivos agrícolas de importancia económica en la región donde el proyecto se inserta así como en el país. Objetivo General: Dada la significación económica del Mal de Río Cuarto en la zona maicera de nuestro país, en la cual se cultiva asimismo sorgo y avena, el presente proyecto intenta aportar conocimientos sobre las afecciones producidas por el virus causal de esta enfermedad.

Transmisión experimental del virus del Mal de Río Cuarto mediante insectos (D. kuschelli) criados en laboratorio

El Mal de Río Cuarto es la enfermedad más importante en el cultivo de maíz, ya que produce severos daños y está muy difundida: en la actualidad ocupa una superficie cercana a 1.000.000 de has. Se han evaluado las pérdidas en plantas severamente afectadas en la zona endémica de la virosis determinándose niveles que oscilaron entre un 20 a un 40% según el período agrícola. El virus afecta otros cultivos tales como sorgo, trigo, avena, mijo, moha de Hungría y centeno además de numerosas malezas pertenecientes a las familias de las Poáceas y Cyperáceas. La morfología de la partícula observada en cortes ultra finos permitió modular la hipótesis de similitud o parentesco con la enfermedad llamada Maize Rough Dwarf (MRDV) presente en el Mediterráneo; trabajos posteriores evidenciaron que tanto MRDV como el virus del Mal de Río Cuarto mostraron 10 bandas típicas de los Fijivirus. La enfermedad se transmite en la naturaleza en forma persistente mediante la especie Dephacodes kuschelli Fennah. Dada la importancia económica de la enfermedad se consideró prioritario lograr la cría y transmisión experimental de la virosis con insectos criados en laboratorio, ya que hasta el momento las transmisiones se llevaban a cabo con insectos provenientes de campo. El cumplimiento de este objetivo de trabajo permitirá el desarrollo de otras actividades tales como multiplicación del inóculo y su mantenimiento para la realización de estudios de caracterización biológica y molecular, purificación del virus, determinación de hospedantes diferenciales que permitirán establecer similitud o diferencias entre aislamientos locales y/o extranjeros, determinación de cultivares tolerantes o resistentes entre otras ventajas.

ETIOLOGÍA E IMPORTANCIA ECONÓMICA DE UNA NUEVA ENFERMEDAD VIRAL DE BATATA EN LA PROVINCIA DE CÓRDOBA

La batata se ubica en el séptimo lugar como cultivo destinado a la alimentación humana, y en el quinto luego de arroz, trigo, maíz y mandioca. Globalmente, existen 8 millones de hectáreas plantadas con batata y, aproximadamente el 95% de esa superficie se ubica en más de un centenar de países en desarrollo. En Argentina, la región pampeana (Buenos Aires, Córdoba y Santa Fe) y el NEA representan el 83% de la superficie plantada. Córdoba y Buenos Aires constituyen las principales provincias productoras. A pesar de su importancia potencial en la alimentación humana y animal, como producto exportable y para industrialización, se viene registrando una marcada reducción en el área cultivada con esta hortícola y, entre las causas más relevantes que determinan este fenómeno, se encuentran las enfermedades virales. Históricamente estas patologías han sido la principal limitante en la producción de este cultivo en Argentina y, especialmente en Córdoba. Recientemente y, tras brindar solución al grave problema ocasionado por el “enanismo clorótico” (Sweet potato chlorotic dwarf disease), virosis que afectó al cv Morada INTA en la década del 90, se observó, en nuestra provincia, la aparición de una severa sintomatología viral en lotes de producción implantados con el cv Arapey INIA, genotipo de creciente difusión en el cultivo por sus buenas características agronómicas. En virtud de dicha sintomatología, se sugiere que en la nueva patología viral se halla involucrado más de un agente etiológico y que la misma produce daños económicos en la producción de Arapey INIA. Por otra parte, la identificación de el/los virus presentes en la nueva patología es el primer eslabón para la búsqueda de resistencia a los mismos. Se supone, además, que, en germoplasma selecto de batata existen fuentes de resistencia a el/los virus involucrados y, que, al menos uno de los agentes patógenos de esta virosis de Arapey INIA, es transmitido por moscas blancas. Se propone, como paso inicial para el control de la nueva etiología: caracterizar biológica, serológica y molecularmente a el/los virus involucrados en ella; preparar reactivos de diagnóstico para los mismos y evaluar la gravedad de esta virosis a través de la estimación de su incidencia, prevalencia y severidad y de los daños que provoca sobre los componentes de rendimiento, en zonas productoras de la provincia de Córdoba. Por otra parte y, debido a que una de las principales formas de control de estas enfermedades es a través del empleo de germoplasma resistente y, considerando que la mayoría de los cultivares comerciales de batata, incluído Arapey INIA poseen escasa variabilidad genética por ser monoclonales, se pretende explorar molecularmente para genes de resistencia en aproximadamente 30 genotipos (clones) promisorios procedentes de la EEA INTA San Pedro ( Bs.As.), empleados como parentales en policruzamientos, además de hacerlo en el genotipo bajo estudio (Arapey INIA).

Search for very high energy Gamma radiation from the Starburst Galaxy IC 342

This thesis describes a search for very high energy (VHE) gamma-ray emission from the starburst galaxy IC 342. The analysis was based on data from the 2003 — 2004 observing season recorded using the Whipple 10-metre imaging atmospheric Cherenkov telescope located on Mount Hopkins in southern Arizona. IC 342 may be classed as a non-blazar type galaxy and to date only a few such galaxies (M 87, Cen A, M 82 and NGC 253) have been detected as VHE gamma-ray sources. Analysis of approximately 24 hours of good quality IC 342 data, consisting entirely of ON/OFF observations, was carried out using a number of methods (standard Supercuts, optimised Supercuts, scaled optimised Supercuts and the multivariate kernel analysis technique). No evidence for TeV gamma-ray emission from IC 342 was found. The significance was 0.6 a with a nominal rate of 0.04 ± 0.06 gamma rays per minute. The flux upper limit above 600 GeV (at 99.9 % confidence) was determined to be 5.5 x 10-8 m-2 s-1, corresponding to 8 % of the Crab Nebula flux in the same energy range.

A Redescription of Riggia paranensis Szidat, 1948 (Isopoda, Cymothoidae) Based on Thirty-two Specimens from Curimatid Fish of Rio de Janeiro, Brazil, with an Emendation of the Genus

Riggia paranensis Szidat, 1948 is redescribed on the basis of 30 female and 2 male specimens collected from the pericardial cavities of the curimatid fish Cyphocarax (= Curimata) gilberti (Quoy & Gaimard). The fishes were caught in the Itabapoana River, State of Rio de Janeiro, southeastern Brazil. The presence of" dwarf" males, as reported by Szidat, was verified. The fusion of the pleonites and pleotelson in adult females was also confirmed. The generic diagnosis was emended to include details of the mouthparts and pleopods

The extraordinarily bright optical afterglow of GRB 991208 and its host galaxy

Observations of the extraordinarily bright optical afterglow (OA) of GRB 991208 started 2.1 d after the event. The flux decay constant of the OA in the R-band is -2.30 +/- 0.07 up to 5 d, which is very likely due to the jet effect, and after that it is followed by a much steeper decay with constant -3.2 +/- 0.2, the fastest one ever seen in a GRB OA. A negative detection in several all-sky films taken simultaneously to the event implies either a previous additional break prior to 2 d after the occurrence of the GRB (as expected from the jet effect). The existence of a second break might indicate a steepening in the electron spectrum or the superposition of two events. Once the afterglow emission vanished, contribution of a bright underlying SN is found, but the light curve is not sufficiently well sampled to rule out a dust echo explanation. Our determination of z = 0.706 indicates that GRB 991208 is at 3.7 Gpc, implying an isotropic energy release of 1.15 x 10E53 erg which may be relaxed by beaming by a factor > 100. Precise astrometry indicates that the GRB coincides within 0.2' with the host galaxy, thus given support to a massive star origin. The absolute magnitude is M_B = -18.2, well below the knee of the galaxy luminosity function and we derive a star-forming rate of 11.5 +/- 7.1 Mo/yr. The quasi-simultaneous broad-band photometric spectral energy distribution of the afterglow is determined 3.5 day after the burst (Dec 12.0) implying a cooling frequency below the optical band, i.e. supporting a jet model with p = -2.30 as the index of the power-law electron distribution.

Two component Emden sphere

The theory of a self-gravitating gas sphere is given. The gravitational field is generated by two components, each of which is an independent isothermal gas. Various quantities of interest, such as density profiles, core radii of both components, masses, free-free luminosity, surface brightness, central surface density, and overestimate of central mass density, are given for different values of both parameters which arise naturally (ratio of central densities, ratio of rms velocities). Fundamental changes appear when comparison is made with a theory in which the second component is a 'test component'. Procedures are given for the complete analysis of real astrophysical configurations such as clusters of galaxies or globular clusters.

Possible hot spots excited by the relativistic jets of Cygnus X-3

We present the results of a deep search for associated radio features in the vicinity of the microquasar Cygnus X-3. The motivation behind is to find out evidence for interaction between its relativistic jets and the surrounding interstellar medium, which could eventually allow us to perform calorimetry of the total energy released by this microquasar during its flaring lifetime. Remarkably, two radio sources with mJy emission level at centimeter wavelengths have been detected in excellent alignment with the position angle of the inner radio jets. We propose that these objects could be the hot spots where the relativitic outflow collides with the ambient gas in analogy with Fanaroff-Riley II radio galaxies. These candidate hot spots are within a few arc-minutes of Cygnus X-3 and, if physically related, the full linear extent of the jet would reach tens of parsecs. We discuss here the evidence currently available to support this hypothesis based on both archival data and our own observations.

The red island and the seven dwarfs: body size reduction in Cheirogaleidae

AimSmall body size in Madagascar's dwarf and mouse lemurs (Cheirogaleidae) is generally viewed as primitive. We investigated the evolution of body size in this family and in its sister-taxon, the Lepilemuridae, from phylogenetic, ontogenetic and adaptive perspectives. LocationMadagascar. MethodsWe used a phylogenetic method to reconstruct the evolution of body size in lemurs, and allometric regression models of gestation periods and static and growth allometries in Cheirogaleidae and Lepilemuridae to test the hypothesis that dwarfing occurred as a result of truncated ontogeny (progenesis). We also examined adaptive hypotheses relating body size to environmental variability, life history, seasonality of reproduction, hypothermy (use of torpor), and a diet rich in plant exudates. ResultsOur results indicated that cheirogaleids experienced at least four independent events of body size reduction from an ancestor as large as living Lepilemuridae, by means of progenesis. Our interpretation is supported by the paedomorphic appearance and parallel ontogenetic trajectories of the dwarf taxa, as well as their very short gestation periods and increased fecundity. Lepilemur species that occupy more predictable environments are significantly larger than those occupying unpredictable habitats. Main conclusionsCheirogaleidae appear to be paedomorphic dwarfs, a consequence of progenesis, probably as an adaptation to high environmental unpredictability. Although the capacity to use hypothermy is related to small body size, this advantage is unlikely to have driven dwarfing in cheirogaleids. We propose that gummmivory/exudativory co-evolved with body size reduction in this clade, probably from a folivorous ancestor. Their small size is derived, and their suitability as models for the ancestral primate' is therefore dubious.

Kasvillisuuden ja maanmuokkauksen vaikutus männyn ja koivun taimettumiseen varpu- ja puolukkaturvekankailla

Summary: Effect of vegetation and site preparation on the restocking of Scots pine and birch in dwarf-schrub and Vaccinium vitis-idaea type peatland forests

Taxonomic status of Hylomys parvus and Hylomys suillus (Insectivora: Erinaceidae): biochemical and morphological analyses

The genus Hylomys was thought to be represented by a single widespread species. Biochemical and morphometric analyses of several Southeast Asian populations reveal that Sumatra is inhabited by two distinct species, the dwarf gymnure (H. parvus) and the lesser gymnure (H. suillus). The absence of interbreeding between these two groups along with their relatively ancient common origins are documented by several diagnostic loci and a large Nei's genetic distance (D = 0.353 +/- 0.035). The dwarf gymnure has been reported only from the slopes of the Mt. Kerinci volcano in Sumatra, where the species lives at higher elevations than its potential competitor, the lesser gymnure. Other populations of Hylomys from Java, Borneo, and Malaysia are more closely related to the Sumatran sample of H. suillus, but they exhibit strong interpopulational genetic differentiation (D = 0.165 +/- 0.040) that may be accounted for by their isolated montane habitat. In addition, a principal-components analysis based on 16 measurements of the skull clearly separates adult specimens of both species. There is little overlap in the measurements between H. suillus (which is larger) and H. parvus. On Sumatra where both species may be sympatric, the notched space between premaxillary tips, soft texture of the fur, and more delicate skull and dentition are diagnostic of H. parvus.