148 research outputs found

    External Use of Propolis for Oral, Skin, and Genital Diseases: A Systematic Review and Meta-Analysis

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    Objective. The aim of this review is to provide the available evidence on the external use of propolis (EUP) for oral, skin, and genital diseases. Method. We searched twelve electronic databases for relevant studies up to June 2016. Randomized clinical trials (RCTs) were included and analysed. Results. Of the 286 articles identified, twelve potentially relevant studies met our inclusion criteria. A meta-analysis of two studies on recurrent oral aphthae (ROA) indicated that there were no significant differences in total effective rate (TER) for pain disappearance between EUP and placebo groups (RR = 1.96, 95% CI = 0.97–3.98, and P=0.06). In two studies on skin diseases, the combined treatment of EUP with other interventions revealed significant effects on the duration of treatment or TER. In one study on genital diseases, EUP showed significant differences in genital herpes outcome measures compared to placebo. Conclusions. Our results on the effectiveness of EUP for treating oral, skin, and genital diseases are not conclusive because of the low methodological qualities and small sample sizes. Further well-designed randomized controlled trials, with high quality and large samples for specific disorders, must be conducted to obtain firm conclusions

    Nuclear starburst activity induced by elongated bulges in spiral galaxies

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    We study the effects of bulge elongation on the star formation activity in the centers of spiral galaxies using the data from the Sloan Digital Sky Survey Data Release 7. We construct a volume-limited sample of face-on spiral galaxies with Mr<−M_r < -19.5 mag at 0.02 ≀z<\leq z < 0.055 by excluding barred galaxies, where the aperture of the SDSS spectroscopic fibre covers the bulges of the galaxies. We adopt the ellipticity of bulges measured by Simard et al. (2011) who performed two-dimensional bulge+disc decompositions using the SDSS images of galaxies, and identify nuclear starbursts using the fibre specific star formation rates derived from the SDSS spectra. We find a statistically significant correlation between bulge elongation and nuclear starbursts in the sense that the fraction of nuclear starbursts increases with bulge elongation. This correlation is more prominent for fainter and redder galaxies, which exhibit higher ratios of elongated bulges. We find no significant environmental dependence of the correlation between bulge elongation and nuclear starbursts. These results suggest that non-axisymmetric bulges can efficiently feed the gas into the centre of galaxies to trigger nuclear starburst activity.Comment: 9 pages, 7 figures, accepted for publication in MNRA

    Exploration of New Electroacupuncture Needle Material

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    Background. Electro Acupuncture (EA) uses the acupuncture needle as an electrode to apply low-frequency stimulation. For its safe operation, it is essential to prevent any corrosion of the acupuncture needle. Objective. The aim of this study is to find an available material and determine the possibility of producing a standard EA needle that is biocompatible. Methods. Biocompatibility was tested by an MTT assay and cytotoxicity testing. Corrosion was observed with a scanning electron microscope (SEM) after 0.5 mA, 60 min stimulation. The straightness was measured using a gap length of 100 mm, and tensile testing was performed by imposing a maximum tensile load. Results. Phosphor bronze, Ni coated SS304, were deemed inappropriate materials because of mild-to-moderate cytotoxicity and corrosion. Ti-6Al-4V and SS316 showed no cytotoxicity or corrosion. Ti-6Al-4V has a 70 times higher cost and 2.5 times lower conductivity than SS316. The results of both straightness and tensile testing confirmed that SS316 can be manufactured as a standard product. Conclusion. As a result, we confirmed that SS316 can be used a new EA electrode material. We hope that a further study of the maximum capacity of low-frequency stimulation using an SS316 for safe operation

    Freshwater and Terrestrial Algae from Ny-Ålesund and Blomstrandhalvþya Island (Svalbard)

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    A field survey of algae and cyanobacteria from terrestrial and freshwater habitats in the vicinity of Ny-Ålesund and on BlomstrandhalvĂžya Island (Svalbard) was performed in June 2009, and results were compared with data from our fieldwork in June 2006. In total, we identified 30 taxa belonging to 23 genera from the specimens collected near Ny-Ålesund (26 taxa) and on BlomstrandhalvĂžya Island (24 taxa). Five species previously unrecorded from this locality are depicted, including astaxanthin-containing Haematococcus sp. collected from BlomstrandhalvĂžya Island. This is the first report on a Haematococcus species from the High Arctic.Une Ă©tude sur le terrain portant sur les algues et les cyanobactĂ©ries d’habitats terrestres et dulçaquicoles dans les environs de Ny-Ålesund et de l’üle BlomstrandhalvĂžya (Svalbard) a Ă©tĂ© rĂ©alisĂ©e en juin 2009, et les rĂ©sultats ont Ă©tĂ© comparĂ©s aux donnĂ©es de notre travail sur le terrain effectuĂ© en juin 2006. En tout, nous avons identifiĂ© 30 taxons appartenant Ă  23 genres Ă  partir de spĂ©cimens prĂ©levĂ©s prĂšs de Ny-Ålesund (26 taxons) et de BlomstrandhalvĂžya (24 taxons). Cinq espĂšces qui n’avaient jamais Ă©tĂ© rĂ©pertoriĂ©es dans cette localitĂ© sont illustrĂ©es, dont l’Haematococcus sp. contenant de l’astaxanthine recueillie Ă  l’üle BlomstrandhalvĂžya. Il s’agit de la premiĂšre fois que l’espĂšce Haematococcus a Ă©tĂ© signalĂ©e dans l’ExtrĂȘme-Arctique

    Dependence of Barred Galaxy Fraction on Galaxy Properties and Environment

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    We investigate the dependence of occurrence of bars in galaxies on galaxy properties and environment. We use a volume-limited sample of 33,391 galaxies brighter than Mr=−19.5+5M_{r}=-19.5+5loghh at 0.02≀z≀0.054890.02\le z\le0.05489, drawn from the SDSS DR 7. We classify the galaxies into early and late types, and identify bars by visual inspection. Among 10,674 late-type galaxies with axis ratio b/a>0.60b/a>0.60, we find 3,240 barred galaxies (fbar=30.4f_{bar}=30.4%) which divide into 2,542 strong bars (fSB1=23.8f_{SB1}=23.8%) and 698 weak bars (fSB2=6.5f_{SB2}=6.5%). We find that fSB1f_{SB1} increases as u−ru-r color becomes redder, and that it has a maximum value at intermediate velocity dispersion (σ≃\sigma\simeq150 km s−1^{-1}). This trend suggests that strong bars are dominantly hosted by intermediate-mass systems. Weak bars prefer bluer galaxies with lower mass and lower concentration. In the case of strong bars, their dependence on the concentration index appears only for massive galaxies with σ>150\sigma>150 km s−1^{-1}. We also find that fbarf_{bar} does not directly depend on the large-scale background density when other physical parameters (u−ru-r color or σ\sigma) are fixed. We discover that fSB1f_{SB1} decreases as the separation to the nearest neighbor galaxy becomes smaller than 0.1 times the virial radius of the neighbor regardless of neighbor's morphology. These results imply that strong bars are likely to be destroyed during strong tidal interactions, and that the mechanism for this phenomenon is gravitational and not hydrodynamical. The fraction of weak bars has no correlation with environmental parameters. We do not find any direct evidence for environmental stimulation of bar formation.Comment: 20 pages, 18 figures, accepted for publication in Ap
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