1,653 research outputs found

    Young stars and dust in AFGL437: NICMOS/HST polarimetric imaging of an outflow source

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    We present near infrared broad band and polarimetric images of the compact star forming cluster AFGL437 obtained with the NICMOS instrument aboard HST. Our high resolution images reveal a well collimated bipolar reflection nebulosity in the cluster and allow us to identify WK34 as the illuminating source. The scattered light in the bipolar nebulosity centered on this source is very highly polarized (up to 79%). Such high levels of polarization implies a distribution of dust grains lacking large grains, contrary to the usual dust models of dark clouds. We discuss the geometry of the dust distribution giving rise to the bipolar reflection nebulosity and make mass estimates for the underlying scattering material. We find that the most likely inclination of the bipolar nebulosity, south lobe inclined towards Earth, is consistent with the inclination of the large scale CO molecular outflow associated with the cluster, strengthening the identification of WK34 as the source powering it.Comment: 26 pages, 10 figues. Accepted for publication in the Astrophysical Journa

    Efficiency tests of a twenty horse-power Avery Traction Engine no. 2116

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    Citation: Carnahan, August Belmont, Barnard, Asa William, and Thompson, Roger S. Efficiency tests of a twenty horse-power Avery Traction Engine no. 2116. Senior thesis, Kansas State Agricultural College, 1905.Morse Department of Special CollectionsIntroduction: Purpose: The purpose of the following is to set forth the mechanical efficiency of the Avery traction engine No. 2116, running as a stationary engine and as a traction engine; to determine the evaporative power of the boiler under a reasonable load While being fired with Lansing coal from the Kansas Penitentiary; and to determine the draft per ton of haul over dirt and macadamized roads with an ordinary four inch wagon. The instruments used for the tests for mechanical efficiency were: Two Crosby indicators, each closely connected A Crosby disk revolution counter/ A Prony brake/ A platform scale and/ An indicator reducing motion/ To make a reliable test of an engine requires a correct application of instruments and a skillful manipulation of the same. The error of every instrument should be determined before and after the test and necessary corrections made for the same. No instrument of doubtful reading should be used under any circumstances. Ease of manipulation adds much to the accuracy with *high a reading may be made. All readings ought to be made simultaneously in order that they may harmonize. The Indicators: Of the sources of error accompanying the use of indicators we found that two above all should be sought out

    Green and brown bridges between weeds and crops reveal novel Diaporthe species in Australia

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    Diaporthe (syn. Phomopsis) species are well-known saprobes, endophytes or pathogens on a range of plants. Several species have wide host ranges and multiple species may sometimes colonise the same host species. This study describes eight novel Diaporthe species isolated from live and/or dead tissue from the broad acre crops lupin, maize, mungbean, soybean and sunflower, and associated weed species in Queensland and New South Wales, as well as the environmental weed bitou bush (Chrysanthemoides monilifera subsp. rotundata) in eastern Australia. The new taxa are differentiated on the basis of morphology and DNA sequence analyses based on the nuclear ribosomal internal transcribed spacer region, and part of the translation elongation factor-1α and ß-tubulin genes. The possible agricultural significance of live weeds and crop residues ('green bridges') as well as dead weeds and crop residues ('brown bridges') in aiding survival of the newly described Diaporthe species is discussed

    Use of ETC-1002 to treat hypercholesterolemia in patients with statin intolerance

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    BackgroundOnce-daily, oral ETC-1002 reduces low-density lipoprotein cholesterol (LDL-C) and has beneficial effects on other cardiometabolic risk factors but has not been examined in statin intolerant patients.ObjectivesTo study the efficacy and safety of ETC-1002 (a novel LDL-C–lowering agent) in patients with hypercholesterolemia and a history of statin intolerance.MethodsPatients intolerant to at least 1 statin were entered into this multicenter, double-blind, 8-week trial. Participants were required to have a history of muscle complaints that developed during statin treatment and resolved within 4 weeks of statin discontinuation. Patients (n = 56) were randomized in a 2:1 ratio to ETC-1002 60 mg daily or placebo. The ETC-1002 dose was increased at 2-week intervals to 120 mg, 180 mg, and 240 mg. The primary end point was the percentage change from baseline to week 8 in calculated LDL-C.ResultsETC-1002 reduced LDL-C 28.7% more than placebo (95% confidence interval, −35.4 to −22.1; P < .0001). ETC-1002 significantly reduced non–high-density lipoprotein cholesterol, total cholesterol, apolipoprotein B, and high-sensitivity C-reactive protein. Triglycerides and high-density lipoprotein cholesterol did not change with ETC-1002 treatment. Sixty-two percent of patients receiving ETC-1002 and none in the placebo group achieved the 2004 National Cholesterol Education Program Adult Treatment Panel III LDL-C goal (P < .0001). Muscle-related adverse events occurred with similar frequency in the placebo and ETC-1002 treatment groups, causing no discontinuations in ETC-1002–treated patients.ConclusionsETC-1002 appears to be effective at reducing LDL-C and was well tolerated in patients with statin-associated muscle complaints. Longer and larger studies are required to confirm the absence of muscle side effects

    A Study of the Diverse T Dwarf Population Revealed by WISE

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    We report the discovery of 87 new T dwarfs uncovered with the Wide-field Infrared Survey Explorer (WISE) and three brown dwarfs with extremely red near-infrared colors that exhibit characteristics of both L and T dwarfs. Two of the new T dwarfs are likely binaries with L7+/-1 primaries and mid-type T secondaries. In addition, our follow-up program has confirmed 10 previously identified T dwarfs and four photometrically-selected L and T dwarf candidates in the literature. This sample, along with the previous WISE discoveries, triples the number of known brown dwarfs with spectral types later than T5. Using the WISE All-Sky Source Catalog we present updated color-color and color-type diagrams for all the WISE-discovered T and Y dwarfs. Near-infrared spectra of the new discoveries are presented, along with spectral classifications. To accommodate later T dwarfs we have modified the integrated flux method of determining spectral indices to instead use the median flux. Furthermore, a newly defined J-narrow index differentiates the early-type Y dwarfs from late-type T dwarfs based on the J-band continuum slope. The K/J indices for this expanded sample show that 32% of late-type T dwarfs have suppressed K-band flux and are blue relative to the spectral standards, while only 11% are redder than the standards. Comparison of the Y/J and K/J index to models suggests diverse atmospheric conditions and supports the possible re-emergence of clouds after the L/T transition. We also discuss peculiar brown dwarfs and candidates that were found not to be substellar, including two Young Stellar Objects and two Active Galactic Nuclei. The coolest WISE-discovered brown dwarfs are the closest of their type and will remain the only sample of their kind for many years to come.Comment: Accepted to ApJS on 15 January 2013; 99 pages in preprint format, 30 figures, 12 table

    Treatment with ETC-1002 alone and in combination with ezetimibe lowers LDL cholesterol in hypercholesterolemic patients with or without statin intolerance

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    BackgroundETC-1002 is an oral, once-daily, first-in-class medication being developed to treat hypercholesterolemia.ObjectivesTo compare 2 doses of ETC-1002, alone or combined with ezetimibe 10 mg (EZE), vs EZE monotherapy for lowering low-density lipoprotein cholesterol (LDL-C).MethodsThis phase 2b, multicenter, double-blind trial-evaluated hypercholesterolemic patients (LDL-C, 130 to 220 mg/dL) with (n = 177) or without (n = 171) muscle-related intolerance to ≥2 statins; 1 at lowest approved dose. Subjects were randomized to 12-week treatment with ETC-1002 120 mg or ETC-1002 180 mg alone, EZE alone, ETC-1002 120 mg plus EZE, or ETC-1002 180 mg plus EZE.ResultsEZE alone lowered LDL-C by 21%, whereas ETC-1002 monotherapy with 120 mg or 180 mg reduced LDL-C by 27% (P = .0008 vs EZE) and 30% (P < .0001 vs EZE), respectively. The combination of ETC-1002, 120 mg or 180 mg plus EZE reduced LDL-C by 43% and 48%, respectively (both P < .0001 vs EZE). ETC-1002 alone or combined with EZE also reduced non–high-density lipoprotein cholesterol, total cholesterol, apolipoprotein B, LDL particle number, and high-sensitivity C-reactive protein compared with EZE alone. Across all treatment groups, statin-intolerant patients reported more muscle-related adverse events than did statin-tolerant patients. ETC-1002 was safe and well tolerated, and rates of muscle-related adverse events were similar in all treatment groups.ConclusionsIn patients with and without statin intolerance, daily treatment with ETC-1002 120 mg and 180 mg alone or with EZE reduced LDL-C more than EZE alone and had a similar tolerability profile (NCT01941836)

    Measurement of two-halo neutron transfer reaction p(11^{11}Li,9^{9}Li)t at 3AA MeV

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    The p(\nuc{11}{Li},\nuc{9}{Li})t reaction has been studied for the first time at an incident energy of 3AA MeV delivered by the new ISAC-2 facility at TRIUMF. An active target detector MAYA, build at GANIL, was used for the measurement. The differential cross sectionshave been determined for transitions to the \nuc{9}{Li} ground andthe first excited states in a wide range of scattering angles. Multistep transfer calculations using different \nuc{11}{Li} model wave functions, shows that wave functions with strong correlations between the halo neutrons are the most successful in reproducing the observation.Comment: 6 pages, 3 figures, submitted to Physical Review Letter
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