1,078 research outputs found

    Doomed drones? Using passage experiments and mathematical modelling to determine Deformed wing virus population dynamics in male honey bees

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    Funding: This research was funded by the BBSRC (Biotechnology and Biological Sciences Research Council), grant numbers: BB/M010996/1 and BB/R00305X/1. P.C.S was supported by the BBSRC, grant number: BB/S00243X/1.Varroa destructor is an ectoparasitic mite of honeybees which vectors a range of pathogenic viruses, the most notable being Deformed wing virus (DWV). Mites parasitise bees during pupal development and male honeybees, drones, have a longer development cycle than female workers (24 versus 21 days), allow for more progeny mites to develop per foundress (1.6ā€“2.5 compared to 0.7ā€“1.45). How this longer exposure time influences evolution of the transmitted virus population is unknown. Using uniquely tagged viruses recovered from cDNA we investigated the replication, competition and morbidity of DWV genotypes in drones. Assays examining virus replication and morbidity revealed drones are highly susceptible to both predominant genotypes of DWV. In virus passage studies using an equimolar inocula of major DNA genotypes and their recombinants, the recombinant form dominated but did not reach 100% of the virus population within 10 passages. Using an in-silico model of the virusā€“miteā€“bee system we examined bottlenecks during virus acquisition by the mite and subsequent injection of viruses into the host, which may play a significant role in shaping virus diversity. This study furthers our understanding of the variables influencing DWV diversity changes and provides insight into areas of future research in the miteā€“virusā€“bee system.Publisher PDFPeer reviewe

    Managing hostile subsoils in the high rainfall zone of south-western Australia

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    This report is designed to complement existing information on the management of crops in the High Rainfall Zone of south-western Australia and to identify limitations for crop production arising from the soil properties in this area

    The Mid-infrared Evolution of the FU Orionis Disk

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    We present new SOFIA-FORCAST observations obtained in 2016 February of the archetypal outbursting low-mass young stellar object FU Orionis, and we compare the continuum, solid-state, and gas properties with mid-infrared data obtained at the same wavelengths in 2004 with Spitzer-IRS. In this study, we conduct the first mid-infrared spectroscopic comparison of an FUor over a long time period. Over a 12-year period, UBVR monitoring indicates that FU Orionis has continued its steady decrease in overall brightness by ~14%. We find that this decrease in luminosity occurs only at wavelengths ā‰¾20 Ī¼m. In particular, the continuum shortward of the silicate emission complex at 10 Ī¼m exhibits a ~12% (~3Ļƒ) drop in flux density but no apparent change in slope; both the Spitzer and SOFIA spectra are consistent with a 7200 K blackbody. Additionally, the detection of water absorption is consistent with the Spitzer spectrum. The silicate emission feature at 10 Ī¼m continues to be consistent with unprocessed grains, unchanged over 12 years. We conclude that either the accretion rate in FU Orionis has decreased by ~12ā€“14% over this time baseline or the inner disk has cooled, but the accretion disk remains in a superheated state outside the innermost region
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