OIL VALUE VARIATIONS AND COST-EFFECTIVENESS TOWARDS WEALTH CREATION OF OIL AND GAS VENDING CORPORATIONS

The study investigated the effect of oil value variations and cost-effectiveness towards wealth creation of oil and gas vending corporations. The main objective of the study was to determine whether oil value variation impact on cost-effectiveness in the processes of wealth creation in oil and gas vending corporations in Nigeria. Data were obtained from secondary sources such as annual financial reports of corporations which were within the coverage years of investigation. Simple regression technique was used to analyze the data collected. The findings revealed that, oil value variations do not significantly affect cost-effectiveness in the processes of wealth creation of oil and gas vending corporations under consideration. Based on the findings, the study recommended that the management of companies should devise effective strategies in regulating and controlling the effect of oil value variations on their corporate cost-effectiveness towards wealth creation. JEL: L20; L22; L72  Article visualizations

CHARTERING FUNDING AND RETURN ON ASSETS OF GUARANTEE CURRENCY STORES

The study set out to examine the chartering funding and return on assets of Guarantee Currency Stores. The study adopted the ex-post facto research design. The main purpose of the study was to generally evaluate the extent to which chartering funding could be considered as a better option amongst the various options of funding and extent which chartering funding affect the return on assets of guarantee currency stores. Data were collected from the annual reports of the selected Guarantee Currency Stores and the data were analyzed using regression method. The findings revealed that there is positive and significant relationship between funding charter, debt funding and return on asset respectively. Based on the findings, it was concluded that funding charter is one of the major sources of funding any asset as this option of funding ensures ample return on asset. The policy and economic implications are that; Guarantee Currency Stores should think through and judiciously appraise funding charter alternative in the construction of their capital structure as this increases return on asset more than others sources of capital while Machinery Charter Union of Nigeria should create more awareness on the significance of funding charter to encourage those Guarantee Currency Stores seeking for funds to use either funding charter or debt capital taking into reflection the benefits of the two options in terms of improved corporate return on asset.  Article visualizations

Multiband Comparative Study of Optical Microvariability in RL vs. RQ Quasars

We present the results of an optical multi-band (BVR) photometric monitoring program of 22 core-dominated radio-loud quasars (CRLQs) and 22 radio-quiet quasars (RQQs). The aim was to compare the properties of microvariability in both types of quasars. We detected optical microvariability in 5 RQQs and 4 CRLQs. Our results confirm that microvariability in RQQs may be as frequent as in CRLQs. In addition we compare microvariability duty cycles in different bands. Finally, the implications for the origin of the microvariations are briefly discussed.Comment: 17 pages, 14 figures, Accepted for publication in the Astronomical Journa

Antibacterial Activities of Nepetalactones Against Public Health-Related Pathogens

The antimicrobial activities of (Z,E)- and (E,Z)-nepetalactones, 2 major compositional compounds from the essential oil of catnip (Nepeta cataria), were first discovered from fly larval development media studies with over 98% inhibition of bacterial growth. Further investigation demonstrated inhibition of the growth of various bacterial species of public health significance. Catnip oil showed antibacterial activity against 5 Gram-positive and 9 Gram-negative bacteria. The antimicrobial activity varied among the original essential oil from the plant and its major compositional compounds as a blended mixture or an individual compound. Growth inhibition was observed against 5 Neisseria species, with particularly strong inhibition against Neisseria sicca (with MICs ranging from 0.5 to 5 mg/mL) that provided comparable or increased levels of growth control produced by 2 antibiotics (Ceftiofur and Cephalothin). The development of plant-based antibacterial agents to prevent or delay the emergence of antimicrobial resistance in bacteria is discussed

Targeted alveo-pleural fistula endobronchial valve treatment using ventilation scintigraphy

Persistent air-leaks can be difficult to localize in radiology. Bronchoscopic management of air-leaks requires identification of the leak\u27s location to allow suitable targeted treatment. One-way endobronchial valves have become a suitable option for persistent air-leaks. In this report, a combination scintigraphy and one-way endobronchial valve treatment successfully resolved a persistent air-leak

The Transit Light Curve Project. V. System Parameters and Stellar Rotation Period of HD 189733

We present photometry of HD 189733 during eight transits of its close-in giant planet, and out-of-transit photometry spanning two years. Using the transit photometry, we determine the stellar and planetary radii and the photometric ephemeris. Outside of transits, there are quasiperiodic flux variations with a 13.4 day period that we attribute to stellar rotation. In combination with previous results, we derive upper limits on the orbital eccentricity, and on the true angle between the stellar rotation axis and planetary orbit (as opposed to the angle between the projections of those axes on the sky).Comment: Accepted for publication in AJ [21 pages]; minor change

Reverberation Measurements of the Inner Radius of the Dust Torus in Nearby Seyfert 1 Galaxies

The most intense monitoring observations yet made in the optical (UBV) and near-infrared (JHK) wave bands were carried out for nearby Seyfert1 galaxies of NGC 5548, NGC 4051, NGC 3227, and NGC 7469. Over three years of observations with MAGNUM telescope since early 2001, clear time-delayed response of the K-band flux variations to the V-band flux variations was detected for all of these galaxies. Their H-K color temperature was estimated to be 1500-1800 K from the observed flux variation gradients, which supports a view that the bulk of the K flux should originate in the thermal radiation of hot dust that surrounds the central engine. Cross-correlation analysis was performed to quantify the lag time corresponding to the light-travel distance of the hot dust region from the central engine. The measured lag time is 47-53 days for NGC 5548, 11-18 days for NGC 4051, about 20 days for NGC 3227, and 65-87 days for NGC 7469. We found that the lag time is tightly correlated with the optical luminosity as expected from dust reverberation ($\Delta t \propto L^{0.5}$), while only weakly with the central virial mass, which suggests that an inner radius of the dust torus around the active nucleus has a one-to-one correspondence to central luminosity. In the lag time versus central luminosity diagram, the K-band lag times place an upper boundary on the similar lag times of broad-emission lines in the literature. This not only supports the unified scheme of AGNs, but also implies a physical transition from the BLR out to the dust torus that encircles the BLR. Furthermore, our V-band flux variations of NGC 5548 on timescales of up to 10 days are found to correlate with X-ray variations and delay behind them by one or two days, indicating the thermal reprocessing of X-ray emission by the central accretion flow.Comment: ApJ, March 2006, v639 issue, 24 pages, 33 figures, 10 table

Inner Size of a Dust Torus in the Seyfert 1 Galaxy NGC 4151

The most intense monitoring observations yet made were carried out on the Seyfert 1 galaxy NGC 4151 in the optical and near-infrared wave-bands. A lag from the optical light curve to the near-infrared light curve was measured. The lag-time between the V and K light curves at the flux minimum in 2001 was precisely 48+2-3 days, as determined by a cross-correlation analysis. The correlation between the optical luminosity of an active galactic nucleus (AGN) and the lag-time between the UV/optical and the near-infrared light curves is presented for NGC 4151 in combination with previous lag-time measurements of NGC 4151 and other AGNs in the literature. This correlation is interpreted as thermal dust reverberation in an AGN, where the near-infrared emission from an AGN is expected to be the thermal re-radiation from hot dust surrounding the central engine at a radius where the temperature equals to that of the dust sublimation temperature. We find that the inner radius of the dust torus in NGC 4151 is $\sim$ 0.04 pc corresponding to the measured lag-time, well outside the broad line region (BLR) determined by other reverberation studies of the emission lines.Comment: Accepted for publication in ApJ Letters, 13 pages, 3 figures; Corrected typo