4,994 research outputs found

    Line Ratios Reveal N2H+ Emission Originates Above the Midplane in TW Hydrae

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    Line ratios for different transitions of the same molecule have long been used as a probe of gas temperature. Here we use ALMA observations of the N2H+ J~=~1-0 and J~=~4-3 lines in the protoplanetary disk around TW Hya to derive the temperature at which these lines emit. We find an averaged temperature of 39~K with a one sigma uncertainty of 2~K for the radial range 0.8-2'', significantly warmer than the expected midplane temperature beyond 0.5'' in this disk. We conclude that the N2H+ emission in TW Hya is not emitting from near the midplane, but rather from higher in the disk, in a region likely bounded by processes such as photodissociation or chemical reprocessing of CO and N2 rather than freeze out.Comment: Accepted for publication in ApJ Letters, 5 pages, 1 figur

    Survival of Fecal Contamination Indicator Organisms in Soil

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    Soils amended with human or animal waste may result in pathogen contamination of ground and surface water. Because temperature has been shown to affect pathogen survival, two laboratory studies were conducted to evaluate the impact of extremes in temperature on bacterial and viral pathogen indicator die-off in soil. A Captina silt loam was amended with broiler litter (0.1 g/g dry soil), septic tank effluent, or Escherichia coli (ATCC 13706) culture (both at 0.04 and 0.1 mL/g dry soil in the two respective studies), incubated at 5 and 35°C, and analyzed over time to determine the number of fecal coliform, E. coli, and coliphage remaining. Pathogen indicator die-off rate constants (k) for all indicator- temperature-treatment combinations were determined by first-order kinetics. For all three pathogen indicators, die-off was significantly more rapid at 35°C than at 5°C. In both studies, fecal coliform die-off rates were not different from E. coli die-off rates across each temperature-treatment combination. Levels of these bacterial indicators appeared in a ratio of 1:0.94 with 95% confidence intervals at 0.89 and 0.99 in the E. coli- and litter-amended soils. Die-off of the viral indicator was significantly slower than the die-off of the bacterial indicators at 5°C in litter-amended soil. Die-off of the bacterial indicator, E. coli, in soil amended with E. coli culture was not significantly different than die-off in soil amended with broiler litter at 5 or 35°C in the two studies. Because the higher incubation temperature increased die-off rates for all three indicators, it is expected that the potential for contamination of ground and surface water decreases with increasing temperature

    An Archaic-Woodland Site in Calhoun County, S.C., 38CL4

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    https://scholarcommons.sc.edu/archanth_books/1023/thumbnail.jp

    An evaluation of educational media programs in Oklahoma public schools /

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    Health Transfers: An Application of Health-Health Analysis to Assess Food Safety Regulations

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    The authors apply a Health-Health Analysis to risks associated with harvesting Gulf oysters to evaluate that approach to managing health and safety risks

    On the methanol emission detection in the TW Hya disc: the role of grain surface chemistry and non-LTE excitation

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    The recent detection of gas-phase methanol (CH3_3OH) lines in the disc of TW Hya by Walsh et al. provided the first observational constraints on the complex O-bearing organic content in protoplanetary discs. The emission has a ring-like morphology, with a peak at 3050\sim 30-50 au and an inferred column density of 36×1012\sim 3-6\times10^{12} cm2^{-2}. A low CH3_3OH fractional abundance of 0.34×1011\sim 0.3-4\times 10^{-11} (with respect to H2_2) is derived, depending on the assumed vertical location of the CH3_3OH molecular layer. In this study, we use a thermo-chemical model of the TW Hya disc, coupled with the ALCHEMIC gas-grain chemical model, assuming laboratory-motivated, fast diffusivities of the surface molecules to interpret the CH3_3OH detection. Based on this disc model, we performed radiative transfer calculations with the LIME code and simulations of the observations with the CASA simulator. We found that our model allows to reproduce the observations well. The CH3_3OH emission in our model appears as a ring with radius of 60\sim60 au. Synthetic and observed line flux densities are equal within the rms noise level of observations. The synthetic CH3_3OH spectra calculated assuming local thermodynamic equilibrium (LTE) can differ by up to a factor of 3.5 from the non-LTE spectra. For the strongest lines, the differences between LTE and non-LTE flux densities are very small and practically negligible. Variations in the diffusivity of the surface molecules can lead to variations of the CH3_3OH abundance and, therefore, line flux densities by an order of magnitude.Comment: Accepted for publication in MNRAS, 8 pages, 8 figure

    Table of contents and editorial information for Vol. 10, no. 2, Spring 1983

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    Table of contents and editorial information for Vol. 10, no. 2, Spring 198

    Educational Considerations, vol. 10(2) Full Issue

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    Educational Considerations, vol. 10(2) Spring 1983 - Full issu
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