1,726,211 research outputs found
Block Card 5904 Livingston Drive
No full textThis 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 | 5904 Livingston Drive (Toledo, Ohio) | Cape Cod Style | Hopewell Acres (Toledo, Ohio) | Greenwood Area (Toledo, Ohio) | West Toledo Area (Toledo, Ohio
Block Card 5904 Pickard Drive
No full textThis 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 | 5904 Pickard Drive (Toledo, Ohio) | Hopewell Acres (Toledo, Ohio) | Greenwood Area (Toledo, Ohio) | West Toledo Area (Toledo, Ohio) | Folk House Styl
Block Card 5904 Foth Drive
No full textThis 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 Style | 5904 Foth Avenue (Toledo, Ohio) | Dwelling | Garnet Place Addition (Toledo, Ohio) | Trilby Area (Toledo, Ohio)
Block Card 5904 Davida Drive
No full textThis 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 | 5904 Davida Drive (Toledo, Ohio) | Ranch houses | North Toledo (Toledo, Ohio) | Greenwood Area (Toledo, Ohio) | Davida Park (Toledo, Ohio
Studi penentuan usia gugus bola NGC 5904 melalui isochrone fitting
Full text linkPenelitian ini dilakukan untuk mengukur usia gugus bola NGC 5904 yang diperoleh melalui isochrone fitting berdasarkan data fotometri GAIA EDR3 dan data keanggotaan gugus bola yang dibuat oleh Baumgardt dan Hilker. Model isochrone
dibangun menggunakan tabel isochrone yang diperoleh dari The MESA Isochrones and Stellar Track dengan berbagai variasi parameter metalisitas, ekstingsi, dan usia. Usia gugus bola kemudian dapat diperoleh dengan membandingkan color magnitude diagram data dan color magnitude diagram model menggunakan metode Least Square. Hasil yang diperoleh dari penelitian ini adalah usia gugus bola NGC 5904 sebesar 11,8 miliar tahun dengan reddening Ev = 0,0035
Block Card 5904 Holly Glenn Drive
No full textThis 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 | 5904 Holly Glenn Drive (Toledo, Ohio) | Cape Cod Style | North Toledo Area (Toledo, Ohio) | Greenwood Area (Toledo, Ohio) | Benalex Heights (Toledo, Ohio
Block Card 5904 West Benalex Drive
No full textThis 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 | 5904 West Benalex Drive (Toledo, Ohio) | Ranch houses | North Toledo (Toledo, Ohio) | Greenwood Area (Toledo, Ohio) | Benalex Heights (Toledo, Ohio
Optical and X-Ray Studies of Compact X-ray binaries in NGC 5904
Full text linkGlobular clusters are the oldest objects in the Milky Way, serving as probes of early galactic evolution due to their chemically uncontaminated history. Compact binaries act as an internal energy source through their dynamical interactions, and measuring the types of X-ray binaries within a cluster provides an understanding of its stellar population and dynamics, as stellar collisional frequencies have been correlated to the number of X-ray sources detected in globular clusters. Compact binaries can be found by correlating X-ray positional data with optical imaging data. In this project, optical fluxes of sources from archival HST images of NGC 5904 have been measured using a DOLPHOT PSF photometry in the optical and Hydrogen-alpha (H↵). A data analysis pipeline has been developed to process of tens of thousands of objects using Awk, Python and DOLPHOT. We identify potential optical counterparts of X-ray sources detected with the Chandra X-Ray Observatory based on their positions as outliers in color-color diagrams and color-magnitude diagrams. Seven out of nine Chandra X-ray sources within the field of view (FOV) of our HST images of NGC 5904 contain such outliers. Furthermore, X-ray fluxes of the sources in NGC 5904, along with DOLPHOT photometric fluxes are also used to determine the X-ray to optical flux ratio, which is used to identify the types of compact X-ray binaries in NGC 5904. We find four out of seven compact X-ray binaries to be Cataclysmic Variables, two to be Active Binaries, and one to be a Millisecond Pulsar. This provides details of the inner workings of NGC 5904, which has a high number of X-ray sources and a large collision rate. Support for this research from the Illinois Space Grant Consortium is gratefully acknowledged
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