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Astronomische Nachrichten, nos 3102-3116
R. R. Astronomische Nachrichten, nos 3102-3116. In: Bulletin astronomique, tome 9, 1892. pp. 430-440
McConnell, A E, 2/3116
This record was harvested from a previous catalogue system and will be withdrawn in 2025. Information in this record may be superseded or incomplete.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/428210Surname: McConnell. Given Name(s) or Initials: A E. Military Service Number or Last Known Location: 2/3116. Prisoner of War Enquiry Card Index Number: K.99. Division Enquiry: NSW. Rank: PTE. Unit: [No Unit]326966
Item: [2016.0049.60472] "McConnell, A E, 2/3116
Block Card 3116 Villa Drive
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 | 3116 Villa Drive (Toledo, Ohio) | Dwelling | Southern Woods (Toledo, Ohio) | South Toledo Area (Toledo, Ohio
Block Card 3116 Cambridge Street
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: multi-family | Italianate Style | Dwelling | 3116 Cambridge Street (Toledo, Ohio) | Cottage Park Addition (Toledo, Ohio) | Lagrange-Central Area (Toledo, Ohio) | North Toledo (Toledo, Ohio
RELACION de las fiestas con que celebró... Cádiz la venturosa venida de N.N. Amados Soberanos... segun lo anuncia el Suplemento del Correo de Cádiz de 15 de Marzo de 1796.
Hay un ejemplar encuadernado con: NOTICIA puntual de la real comitiva que va sirviendo á SS.MM. y AA. en su Viage desde Madrid á Barcelona. (XVIII/3116)Pie de imp. tomado de colofón.Sign. : [calderón]2, 2[calderón]4
Going Beyond Counting First Authors in Author Co-citation Analysis
The present study examines one of the fundamental aspects of author co-citation analysis (ACA) - the way co-citation
counts are defined. Co-citation counting provides the data on which all subsequent statistical analyses and mappings
are based, and we compare ACA results based on two different types of co-citation counting - the traditional type that
only counts the first one among a cited work's authors on the one hand and a non-traditional type that takes into
account the first 5 authors of a cited work on the other hand. Results indicate that the picture produced through this non-traditional author co-citation counting contains more coherent author groups and is therefore considerably clearer. However, this picture represents fewer specialties in the research field being studied than that produced through the traditional first-author co-citation counting when the same number of top-ranked authors is selected and analyzed. Reasons for these effects are discussed
Ragland, Nancy (Stewart), 1861-1948 (SC 3116)
Finding aid and scans (Click on Additional Files below) for Manuscripts Small Collection 3116. Letters, 22 March 1946 and 14 May 1947, of Nancy (Stewart) Ragland, Warren County, Kentucky, to her granddaughter Gwendolyn and her family in Quality, Kentucky, concerning household and family matters. A nephew’s letter of 29 October 1948 describes his attendance at the funeral of “Aunt Nan” and his return home to Arkansas; he refers to several family members by first name only
Possible detection of a cool-core in the cluster RXC J1252.5-3116
This paper presents a detailed study of X-ray emission from the cluster RXC J1252.5-3116, based on an analysis of the Chandra archival data. Here we present radial profiles and maps of X-ray surface-brightness, temperature, electron number density, entropy and pressure of RXC J1252.5-3116. We have also estimated the X-ray luminosity, gas mass, cooling time and mass deposition rate for the cluster. The cluster shows an extremely relaxed X-ray morphology and the radial profiles suggest a drop in the temperature of the central gas. We find an extremely small cool-core and a high mass deposition rate of 43 M⊙ per year. RXC J1252.5-3116 seems to host a possible cool core at its centre
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