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Resolución Rectoral N° 578/2020.Derogar la Resolución Rectoral N° 571/2020.
No full textFil: Rector (R). Universidad Nacional de Río Negro. Río Negro, ArgentinaResolución Rectoral N° 578/2020.Derogar la Resolución Rectoral N° 571/2020.tru
Participant 571 Community Conversations Written Interview
No full textIn this written interview, Participant 571 talks about the challenges they have experienced with job loss, financial instability, and a lack of government resources. The participant says that finances are a constant struggle for their family, but that food donations were an act of kindness they received during the pandemic. The participant shares that social isolation is a source of sadness, and that they are disappointed that their children are not socializing adequately because schools are closed. The participant expresses that they wish all information sources had translation services because sometimes they had to resort to using an online translator to understand COVID-19-related information available on the internet.New Jersey Department of Healt
Verlustliste Nr. 571. (Nr. 571. /1917)
No full textVERLUSTLISTE NR. 571.
Verlustliste (-)
Verlustliste Nr. 571. (Nr. 571. /1917) ([1])
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Offiziere. (3)
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Band 2, 571 (Sammlung Friedlaender)
No full textBAND 2, 571 (SAMMLUNG FRIEDLAENDER)
Band 2, 571 (Sammlung Friedlaender) (Public Domain) (1
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
Searching for an interstellar medium association for HESS J1534-571
Get PDF© 2018 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society. The Galactic supernova remnant HESS J1534-571 (also known as G323.7-1.0) has a shell-like morphology in TeV gamma-ray emission and is a key object in the study of cosmic ray origin. Little is known about its distance and local environment. We examine Mopra 12CO/13CO(1-0) data, Australian Telescope Compact Array HI, and Parkes HI data towards HESS J1534-571. We trace molecular clouds in at least five velocity ranges, including clumpy interstellar medium structures near a dip in HI emission at a kinematic velocity consistent with the Scutum-Crux arm at ~3.5 kpc. This feature may be a cavity blown-out by the progenitor star, a scenario that suggests HESS J1534-571 resulted from a core-collapse event. By employing parametrizations fitted to a sample of supernova remnants of known distance, we find that the radio continuum brightness of HESS J1534-571 is consistent with the ~3.5 kpc kinematic distance of the Scutum-Crux arm HI dip. Modelling of the supernova evolution suggests a ~8-24 kyr age for HESS J1534-571 at this distance
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