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Stain, J C, 2437
No full textThis record was harvested from a previous catalogue system and will be withdrawn in 2025. Information in this record may be superseded or incomplete. Visit this record in UMA's new catalogue at: https://archives.library.unimelb.edu.au/nodes/view/418765Surname: STAIN. Given Name(s) or Initials: J C. Military Service Number or Last Known Location: 2437. Missing, Wounded and Prisoner of War Enquiry Card Index Number: 47594.242754
Item: [2016.0049.51026] "Stain, J C, 2437
Block Card 2437 Dorr Street
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: Shotgun houses | 2437 Dorr Street (Toledo, Ohio) | Dwelling | Scott Park Area (Toledo, Ohio
Block Card 2437 Meadowwood 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: English Cottage Style | 2437 Meadowwood Drive (Toledo, Ohio) | Dwelling | Old Orchard Addition (Toledo, Ohio) | Old Orchard Area (Toledo, Ohio
The open cluster NGC 2437 (Messier 46)
No full textThe stellar content of the open cluster NGC 2437 (Messier 46) is investigated using moderately deep u*, g\u2032, and r\u2032 MegaCam images. When compared with solar metallicity isochrones, the (g\u2032; u\u2032 - g\u2032) and (r\u2032; g\u2032 - r\u2032) CMDs are consistent with an age log(tyr) = 8:35 \ub1 0:15, a distance modulus \u3bc0 = 11:05 \ub1 0:05, and a color excess E(B - V) = 0:115 \ub1 0:035. The r\u2032 luminosity function (LF) of main sequence stars in the magnitude range r\u2032 < 17 (i.e., masses ~0:8 M f) has a shape that follows solar neighborhood star counts. However, at fainter magnitudes, the cluster LF is flat, in contrast with what would be expected from solar neighborhood counts. The clustering properties of stars in NGC 2437 are investigated by examining the two-point angular correlation functions of main sequence stars in different brightness ranges. Main sequence stars fainter than r\u2032 = 17 are less centrally concentrated than brighter stars and are found over a larger area of the sky, suggesting that there is a corona of faint main sequence stars around NGC 2437. Based on the flat LF and extended spatial distribution of faint stars, it is concluded that NGC 2437 is actively shedding stars with masses ~0:8 M f.\ua9 2013. The Astronomical Society of the Pacific. All rights reserved.Peer reviewed: YesNRC publication: Ye
Letras de los villancicos, que se han de cantar en los Solemnes Maytines del Sagrado Nacimiento de Ntro. Redentor Jesuchristo en la Sta. Iglesia Insigne Colegial ... de Antequera
Get PDFHay un ejemplar encuadernado con el volumen facticioXVIII/2437.Port. orlada
Block Card 2437 Greenlawn 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 houses | 2437 Greenlawn Drive (Toledo, Ohio) | Dwelling | Byrne Way Subdivision (Toledo, Ohio) | South Toledo Area (Toledo, Ohio
Letras de los villancicos que se han de cantar en los Solemnes Maytines del Sagrado Nacimiento de N. Redentor Jesu-Christo en la Sta. Iglesia Insigne Colegial ... de Antequera
Get PDFHay un ejemplar encuadernado con el volumen facticioXVIII/2437.Port. orlada.Texto a dos col. y línea tirada
Block Card 2437 Densmore 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: attached garage | Saltbox houses | 2437 Densmore Drive (Toledo, Ohio) | Dwelling | Old Orchard Addition (Toledo, Ohio) | Old Orchard Area (Toledo, Ohio
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