1,724,934 research outputs found

    Comparative Music Education: EDU 4127

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    Examination question paper on Comparative Music education: EDU 4127, Nov 201

    Block Card 4127 East Way

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    This image was produced by the Auditor's Office in Lucas County, Ohio for tax assessment purposes. Associated dates are approximate. Descriptive terms related to this photograph include: Dwelling (Toledo, Ohio) | Cleveland double | Prairie Style | Homeville Subdivision (Toledo, Ohio) | Willys Park area (Toledo, Ohio) | West Toledo (Toledo, Ohio) | 4127 East Way (Toledo, Ohio

    Block Card 4127 Graceway Drive

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    This image was produced by the Auditor's Office in Lucas County, Ohio for tax assessment purposes. Associated dates are approximate. Descriptive terms related to this photograph include: Dwelling – Ohio – Toledo | Ranch Style | Sunnymeade Estates (Toledo, Ohio) | Westgate Area (Toledo, Ohio) | West Toledo (Toledo, Ohio) | 4127 Graceway Drive (Toledo, Ohio

    Block Card 4127 Peak Avenue

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    This image was produced by the Auditor's Office in Lucas County, Ohio for tax assessment purposes. Associated dates are approximate. Descriptive terms related to this photograph include: Dwelling | 4127 Peak Avenue (Toledo, Ohio) | Willys Park Area (Toledo, Ohio) | West Toledo Area (Toledo, Ohio) | Gable front houses | Folk House Styl

    Block Card 4127 Commonwealth Avenue

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    This image was produced by the Auditor's Office in Lucas County, Ohio for tax assessment purposes. Associated dates are approximate. Descriptive terms related to this photograph include: dwelling | multi-family | 4127 Commonwealth Avenue (Toledo, Ohio) | Cleveland double | Craftsman Style | Commonwealth Addition (Toledo, Ohio) | Willys Park area (Toledo, Ohio) | West Toledo (Toledo, Ohio

    Block Card 4127 Patmore Court

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    This image was produced by the Auditor's Office in Lucas County, Ohio for tax assessment purposes. Associated dates are approximate. Descriptive terms related to this photograph include: Ranch houses | Dwelling | Fuller's Mount Vernon Addition (Toledo, Ohio) | Inverness Area (Toledo, Ohio) | 4127 Patmore Court (Toledo, Ohio

    Block Card 4127 Hopkins Court

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    This image was produced by the Auditor's Office in Lucas County, Ohio for tax assessment purposes. Associated dates are approximate. Descriptive terms related to this photograph include: Ranch houses | Dwelling | Fuller's Mount Vernon Addition (Toledo, Ohio) | Inverness Area (Toledo, Ohio) | 4127 Hopkins Court (Toledo, Ohio

    Block Card 4127 Macauley Court

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    This image was produced by the Auditor's Office in Lucas County, Ohio for tax assessment purposes. Associated dates are approximate. Descriptive terms related to this photograph include: Ranch houses | Dwelling | Fuller's Mount Vernon Addition (Toledo, Ohio) | Inverness Area (Toledo, Ohio) | 4127 Macauley Court (Toledo, Ohio

    A High-Eccentricity Warm Jupiter Orbiting TOI-4127

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    International audienceWe report the discovery of TOI-4127 b, which is a transiting, Jupiter-sized exoplanet on a long-period ( P=56.398790.00010+0.00010P={56.39879}_{-0.00010}^{+0.00010} days) and a high-eccentricity orbit around a late F-type dwarf star. This warm Jupiter was first detected and identified as a promising candidate from a search for single-transit signals in TESS Sector 20 data, and was later characterized as a planet following two subsequent transits (TESS Sectors 26 and 53) and follow-up ground-based RV observations with the NEID and SOPHIE spectrographs. We jointly fit the transit and RV data to constrain the physical ( Rp=1.0960.032+0.039RJ{R}_{p}={1.096}_{-0.032}^{+0.039}{R}_{{\rm{J}}} , Mp=2.300.11+0.11MJ{M}_{p}={2.30}_{-0.11}^{+0.11}{M}_{{\rm{J}}} ) and orbital parameters of the exoplanet. Given its high orbital eccentricity ( e=0.74710.0086+0.0078e={0.7471}_{-0.0086}^{+0.0078} ), TOI-4127 b is a compelling candidate for studies of warm Jupiter populations and of hot Jupiter formation pathways. We show that the present periastron separation of TOI-4127 b is too large for high-eccentricity tidal migration to circularize its orbit, and that TOI-4127 b is unlikely to be a hot Jupiter progenitor unless it is undergoing angular momentum exchange with an undetected outer companion. Although we find no evidence for an external companion, the available observational data are insufficient to rule out the presence of a perturber that can excite eccentricity oscillations and facilitate tidal migration
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