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Fraser, Augustus C, 6145
No full textThis record was harvested from a previous catalogue system and will be withdrawn in 2025. Information in this record may be superseded or incomplete.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/386183Surname: FRASER. Given Name(s) or Initials: AUGUSTUS C. Military Service Number or Last Known Location: 6145. Missing, Wounded and Prisoner of War Enquiry Card Index Number: 52382.254248
Item: [2016.0049.18476] "Fraser, Augustus C, 6145
Block Card 6145 Hiddenbrook 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 | 6145 Hiddenbrook Drive (Toledo, Ohio) | Dwelling | Douglas Meadows Addition (Toledo, Ohio) | Trilby Area (Toledo, Ohio)
The Peculiar Filamentary HI Structure of NGC 6145
No full textIn this paper, we report the peculiar H I morphology of the cluster spiral galaxy NGC 6145, which has a 150 kpc H I filament on one side that is nearly parallel to its major axis. This filament is made up of several H I clouds and the diffuse H I gas between them, with no optical counterparts. We compare its H I distribution with other one-sided H I distributions in the literature and find that the overall H I distribution is very different from the typical tidal and ram-pressure stripped H I shape, and that its morphology is inconsistent with that of a pure accretion event. Only similar to 30% of the total H I gas is anchored on the stellar disk, while most of the H I gas forms the filament in the west. At a projected distance of 122 kpc, we find a massive elliptical companion (NGC 6146) with extended radio emission whose axis points to an H I gap in NGC 6145. The velocity of the H I filament shows an overall line-of-sight motion of 80-180 km s(-1) with respect to NGC 6145. Using the long-slit spectra of NGC 6145 along its major stellar axis, we find that some outer regions show enhanced star formation, while in contrast, almost no star formation activities are found in its center (< 2 kpc). Pure accretion, tidal, or ram-pressure stripping are not likely to produce the observed H I filament. An alternative explanation is the jet stripping from NGC 6146, although direct evidence for a jet-cold gas interaction has not been found.Strategic Priority Research Program "The Emergence of Cosmological Structures" of the Chinese Academy of Sciences [XDB09000000]; National Basic Research Program of China (973 Program) [2015CB857004]; National Natural Science Foundation of China (NSFC) [11225315, 1320101002, 11433005, 11421303, 11643001]; Youth Innovation Fund of University of Science and Technology of China [WK2030220019]; Chinese Academy of Sciences through the Hundred Talents Program; National Key Basic Research Program of China [2015CB857004]; NSFC [11173045, 11233005, 11325314, 11320101002]; Strategic Priority Research Program "The Emergence of Cosmological Structures" of CAS [XDB09000000]; Fundamental Research Funds for the Central Universities; National Natural Science Foundation of China [NSFC-11421303]SCI(E)ARTICLE215
E.M. Kaisse, Connected speech : the interaction of syntax and phonology
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Going Beyond Counting First Authors in Author Co-citation Analysis
Get PDFThe 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
Variations on the Author
Get PDF“Variations on the Author” discusses two of Eduardo Coutinho’s recent films (Um Dia na Vida, from 2010, and Últimas Conversas, posthumously released in 2015) and their contribution to the general question of documentary authorship. The director’s filmography is characterized by a consistent yet self-effacing form of authorial self-inscription: Coutinho often features as an interviewer that rather than express opinions propels discourses; an interviewer that is good at listening. This mode of self-inscription characterizes him as an author who is not expressive but who is nonetheless markedly present on the screen. In Um Dia na Vida, however, Coutinho is completely absent form the image, while Últimas Conversas, on the contrary, includes a confessional prologue that moves the director from the margins to the center of his films. This article examines the ways in which these works stand out in the filmography of a director who offers new insights into the notion of cinematic authorship
Appropriate Similarity Measures for Author Cocitation Analysis
Get PDFWe provide a number of new insights into the methodological discussion about author cocitation analysis. We first argue that the use of the Pearson correlation for measuring the similarity between authors’ cocitation profiles is not very satisfactory. We then discuss what kind of similarity measures may be used as an alternative to the Pearson correlation. We consider three similarity measures in particular. One is the well-known cosine. The other two similarity measures have not been used before in the bibliometric literature. Finally, we show by means of an example that our findings have a high practical relevance.information science;Pearson correlation;cosine;similarity measure;author cocitation analysis
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