1,703 research outputs found

    Picking a Fiscal Year, Timing and Nature of Distributions

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    An introductory method for clarinet

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    Thesis (M.A.)--Boston University, 1947. This item was digitized by the Internet Archive

    The Interdisciplinary Music Degree: Music Education, Music Performance, and Music and Fine Arts Administration

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    Despite numerous available careers and degrees in music education, music performance, and music administration, perspectives of many music educators and students desiring an interdisciplinary music degree program inclusive of music education, music performance, and music administration have yet to be expressed or examined publicly. The notion of 21st-century skills presents a demand for flexibility across most facets of K-12 and higher education. These skills necessitate fluency in problem-solving, critical thinking, and collaboration, thus, music education must move toward more flexible and rigorous preparatory music training programs to remain consistent with current trends. Most undergraduate and graduate degree programs in music education, music performance, and music and fine arts administration, however, exist independently, negating the versatility of music degree-seekers through an interdisciplinary music degree. To that end, the researcher designed, examined, and expounded upon existing research pertinent to music educators, performers, and administrators, as well as current, past, and prospective music students, regarding career goals, preparation, and outcomes. This research presents a practical design for an interdisciplinary music degree program across music education, performance, and administration. This study applied a hermeneutic phenomenological qualitative approach, which encourages further analysis by other music researchers that can be applied equally to other fields of music, including music technology, music business, and music therapy. Other fine arts areas like dance, theatre, and visual arts may benefit from similar applications

    Molecule sublimation as a tracer of protostellar accretion: Evidence for accretion bursts from high angular resolution C18O images

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    The accretion histories of embedded protostars are an integral part of descriptions of their physical and chemical evolution. In particular, are the accretion rates smoothly declining from the earlier toward later stages or in fact characterized by variations such as intermittent bursts? We aim to characterize the impact of possible accretion variations in a sample of embedded protostars by measuring the size of the inner regions of their envelopes where CO is sublimated and relate those to their temperature profiles dictated by their current luminosities. Using observations from the Submillimeter Array we measure the extents of the emission from the C18O isotopologue toward 16 deeply embedded protostars. We compare these measurements to the predicted extent of the emission given the current luminosities of the sources through dust and line radiative transfer calculations. Eight out of sixteen sources show more extended C18O emission than predicted by the models. The modeling shows that the likely culprit for these signatures is sublimation due to increases in luminosities of the sources by about a factor five or more during the recent 10,000 years - the time it takes for CO to freeze-out again on dust grains. For four of those sources the increase would have had to have been a factor 10 or more. The compact emission seen toward the other half of the sample suggests that C18O only sublimates when the temperature exceeds 30 K - as one would expect if CO is mixed with H2O in the grain ice-mantles. The small-number statistics from this survey suggest that protostars undergo significant bursts about once every 20,000 years. This also illustrates the importance of taking the physical evolutionary histories into account for descriptions of the chemical structures of embedded protostars.Comment: Accepted by A&A; 11 pages, 5 figure

    Recovery of endurance running capacity: effect of carbohydrate-protein mixtures

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    Including protein in a carbohydrate solution may accelerate both the rate of glycogen storage and the restoration of exercise capacity following prolonged activity. Two studies were undertaken with nine active men in study A and seven in study B. All participants performed 2 trials, each involving a 90 min run at 70% VO2max followed by a 4 h recovery. During recovery, either a 9.3% carbohydrate solution (CHO) or the same solution plus 1.5% protein (CHO-PRO) was ingested every 30 min in volumes providing either 1.2 g CHO · kg-1 · h-1 (study A) or 0.8 g CHO · kg-1 · h-1 (study B). Exercise capacity was then assessed by run time to exhaustion at 85% VO2max. Ingestion of CHO-PRO elicited greater insulinemic responses than CHO (P less than or equal to 0.05) but with no differences in run times to exhaustion. Within the context of this experimental design, CHO and CHO-PRO restored running capacity with equal effect
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