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RISS 인기검색어
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- 저자 : Dale Smith (검색결과 3 건)
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European 1: A globally important clonal complex of Mycobacterium bovis
Smith, N.H.,Berg, S.,Dale, J.,Allen, A.,Rodriguez, S.,Romero, B.,Matos, F.,Ghebremichael, S.,Karoui, C.,Donati, C.,Machado, A.d.C.,Mucavele, C.,Kazwala, R.R.,Hilty, M.,Cadmus, S.,Ngandolo, B.N.R.,Habt Elsevier Science 2011 Infection, genetics and evolution Vol.11 No.6
We have identified a globally important clonal complex of Mycobacterium bovis by deletion analysis of over one thousand strains from over 30 countries. We initially show that over 99% of the strains of M. bovis, the cause of bovine tuberculosis, isolated from cattle in the Republic of Ireland and the UK are closely related and are members of a single clonal complex marked by the deletion of chromosomal region RDEu1 and we named this clonal complex European 1 (Eu1). Eu1 strains were present at less than 14% of French, Portuguese and Spanish isolates of M. bovis but are rare in other mainland European countries and Iran. However, strains of the Eu1 clonal complex were found at high frequency in former trading partners of the UK (USA, South Africa, New Zealand, Australia and Canada). The Americas, with the exception of Brazil, are dominated by the Eu1 clonal complex which was at high frequency in Argentina, Chile, Ecuador and Mexico as well as North America. Eu1 was rare or absent in the African countries surveyed except South Africa. A small sample of strains from Taiwan were non-Eu1 but, surprisingly, isolates from Korea and Kazakhstan were members of the Eu1 clonal complex. The simplest explanation for much of the current distribution of the Eu1 clonal complex is that it was spread in infected cattle, such as Herefords, from the UK to former trading partners, although there is evidence of secondary dispersion since. This is the first identification of a globally dispersed clonal complex M. bovis and indicates that much of the current global distribution of this important veterinary pathogen has resulted from relatively recent International trade in cattle.
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After the Fall: The Dust and Gas in E+A Post-starburst Galaxies
Smercina, A.,Smith, J. D. T.,Dale, D. A.,French, K. D.,Croxall, K. V.,Zhukovska, S.,Togi, A.,Bell, E. F.,Crocker, A. F.,Draine, B. T.,Jarrett, T. H.,Tremonti, C.,Yang, Yujin,Zabludoff, A. I. American Astronomical Society 2018 The Astrophysical journal Vol.855 No.1
<P>The traditional picture of post-starburst galaxies as dust-and gas-poor merger remnants, rapidly transitioning to quiescence, has been recently challenged. Unexpected detections of a significant interstellar medium (ISM) in many post-starburst galaxies raise important questions. Are they truly quiescent, and if so, what mechanisms inhibit further star formation? What processes dominate their ISM energetics? We present an infrared spectroscopic and photometric survey of 33 E+A post-starbursts selected by the Sloan Digital Sky Survey, aimed at resolving these questions. We find compact, warm dust reservoirs with high PAH abundances and total gas and dust masses significantly higher than expected from stellar recycling alone. Both polycyclic aromatic hydrocarbon (PAH)/total infrared (TIR) and dust-to-burst stellar mass ratios are seen to decrease with post-burst age, indicative of the accumulating effects of dust destruction and an incipient transition to hot, early-type ISM properties. Their infrared spectral properties are unique, with dominant PAH emission, very weak nebular lines, unusually strong H-2. rotational emission, and deep [C II] deficits. There is substantial scatter among star formation rate (SFR) indicators, and both PAH and TIR luminosities provide overestimates. Even as potential upper limits, all tracers show that the SFR has typically experienced a decline of more than two orders of magnitude since the starburst and that the SFR is considerably lower than expected given both their stellar masses and molecular gas densities. These results paint a coherent picture of systems in which star formation was, indeed, rapidly truncated, but in which the ISM was not completely expelled, and is instead supported against collapse by latent or continued injection of turbulent or mechanical heating. The resulting aging burst populations provide a 'high-soft' radiation field that seemingly dominates the E+A galaxies' unusual ISM energetics.</P>
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Colonial Legacies and Territorial Claims
Paul R. Hensel,HeeMin Kim,Dale Smith 한국국제정치학회 2008 한국국제정치학회 학술대회 발표논문집 Vol.- No.-
Most of today's nation-states experienced colonial rule at some point during the last two centuries, with well-studied economic, political, and social consequences after decolonization. This study examines a different form of the colonial legacy, involving the stability of the territorial status quo. We lay out a number of different forms that colonial legacies might take with respect to territorial claims, focusing both on relations between two former colonies and on relations between a former colony and its former colonial ruler. We then present and test hypotheses about the impact of these legacies on territorial claims. Our preliminary results show strong evidence that colonial legacies affect territorial conflict after independence, with conflict more likely after violent decolonization and in relations between former colonies of the same colonizer, although more detailed followup research is called for. Paper presented at the conference "National Territory and Sovereignty: Sixty Years Since the Founding of the Nation," Seoul, August 2008. This paper is based on original research by Paul R. Hensel, Michael E. Allison, and Ahmed Khanani. This research was supported by a 2008-2009 grant from the Northeast Asian History Foundation, although the authors retain full responsibility for all content herein; this paper's analyses and conclusions may not necessarily represent the views of the Foundation, the conference organizers, or any other organization.
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