104,940 research outputs found
Advertising Flyer for God\u27s Woman by Charles Ready Nichol, 1938
No full textA flyer advertising Nichols\u27 1938 book, God\u27s Woman published both by Mrs. C. R. Nichol and Wm. B. Eerdmans Publishing Company. This flyer contains testimonials commending the book by some of the most notable evangelists, editors, educators and preachers among Churches of Christ: W. L. Oliphant, T. E. Milholland, G. H. P. Showalter, Leslie G. Thomas, R. L. Whiteside, N. B. Hardeman, Guy N. Woods and Gus Nichols. Nichol\u27s book argued for expanded speaking roles for women in the assembly and deaconesses.https://digitalcommons.acu.edu/sc_teaching_images/1045/thumbnail.jp
G. E. Luck, left, and Major Frederick W. Nichol of New York City, inspecting accounting machine
No full textG. E. Luck, left, and Major Frederick W. Nichol of New York City, inspecting accounting machine.https://mavmatrix.uta.edu/specialcollections_startelegram1940s/14561/thumbnail.jp
Lawrence Walter Nichol 1935-2015
No full textLawrence (Laurie) Walter Nichol FAA was Vice Chancellor of the Australian National University (ANU) from 1988 to 1993, and before that, of the University of New England (UNE) from 1985 to 1988. His independent academic career began in 1963 at the ANU as a Research Fellow in the Department of Physical Biochemistry in the John Curtin School of Medical Research (JCSMR). The department was headed by Professor Alexander (Sandy) G. Ogston FRS. Thus, Laurie's career finally circled back, after overseas sabbaticals and other appointments at Australian universities, to the ANU
Lawrence Walter Nichol 1935-2015
No full textLawrence (Laurie) Walter Nichol FAA was Vice Chancellor of the Australian National University (ANU) from 1988 to 1993, and before that, of the University of New England (UNE) from 1985 to 1988. His independent academic career began in 1963 at the ANU as a Research Fellow in the Department of Physical Biochemistry in the John Curtin School of Medical Research (JCSMR). The department was headed by Professor Alexander (Sandy) G. Ogston FRS. Thus, Laurie’s career finally circled back, after overseas sabbaticals and other appointments at Australian universities, to the ANU
Professor Sargeson, Professor Athelstan Beckwith, Professor Arthur Birch, Professor LW Nichol
No full textResearch School of Chemistry - Dr. Denis Evans, Prof. Alan Sargeson, Mr. Rod Rickards, Prof. Arthur Birch, Prof. Lew Mander, Prof. Stan Athel Beckwith, Prof. L. W. Nichol, Mr. Chris Tomkins, Mr. Gordon G. Lockhart, Dr. John Thompson, Mr. John Harper, Mr. Andrew McMurray & other
Galaxy Zoo:chiral correlation function of galaxy spins
No full textGalaxy Zoo is the first study of nearby galaxies that contains reliable information about the spiral sense of rotation of galaxy arms for a sizeable number of galaxies. We measure the correlation function of spin chirality (the sense in which galaxies appear to be spinning) of face-on spiral galaxies in angular, real and projected spaces. Our results indicate a hint of positive correlation at separations less than ~0.5 Mpc at a statistical significance of 2-3 sigma. This is the first experimental evidence for chiral correlation of spins. Within tidal torque theory it indicates that the inertia tensors of nearby galaxies are correlated. This is complementary to the studies of nearby spin axis correlations that probe the correlations of the tidal field. Theoretical interpretation is made difficult by the small distances at which the correlations are detected, implying that substructure might play a significant role, and our necessary selection of face-on spiral galaxies, rather than a general volume-limited sample
Bibliographie Hilarion G. Petzold 1958 – 2009 mit Anhang als Einführung
No full textDieses Archiv enthält die Gesamtbibliographie der Werke des Autors nebst einiger Texte „Über H. G. Petzold“ im Schlussteil der Bibliographie sowie einen Anhang mit einer Einführung in die Architektur des Werkes in seinem wissenslogischen Aufbau als Ausarbeitung seines „Tree of Science Modells“ (2007).This archive contains the complete bibliography of the author and some texts about H. G. Petzold, moreover an epilogue with an introduction to the architecture of the works in its epistemological structure and composition and as an elaborations of Petzold’s „Tree of Science Modell (2007).https://www.fpi-publikation.de/polyloge/01-2009-petzold-h-g-gesamtbibliographie-h-g-petzold-1958-2009-updating-november2009/peerReviewedpublishedVersio
Dispelling the Myths Behind First-author Citation Counts
No full textWe conducted a full-scale evaluative citation analysis study of scholars in the XML research field to explore just how different from each other author rankings resulting from different citation counting methods actually are, and to demonstrate the capability of emerging data and tools on the Web in supporting more realistic citation counting methods. Our results contest some common arguments for the continued
use of first-author citation counts in the evaluation of scholars, such as high correlations between author rankings by first-author citation counts and other citation
counting methods, and high costs of using more realistic citation counting methods that are not well-supported by the ISI databases. It is argued that increasingly available digital full text research papers make it possible for citation analysis studies to go beyond what the ISI databases have directly supported and to employ more
sophisticated methods
Mr Gordon G Lockhart
No full textResearch School of Chemistry - Dr. Denis Evans, Prof. Alan Sargeson, Mr. Rod Rickards, Prof. Arthur Birch, Prof. Lew Mander, Prof. Stan Athel Beckwith, Prof. L. W. Nichol, Mr. Chris Tomkins, Mr. Gordon G. Lockhart, Dr. John Thompson, Mr. John Harper, Mr. Andrew McMurray & other
From star‐forming spirals to passive spheroids: integral field spectroscopy of E+A galaxies
No full textWe present three‐dimensional spectroscopy of 11 E+A galaxies at z = 0.06–0.12. These galaxies were selected for their strong Hδ absorption but weak (or non‐existent) [O ii ] λ3727 and Hα emission. This selection suggests that a recent burst of star formation was triggered but subsequently abruptly ended. We probe the spatial and spectral properties of both the young (≲1 Gyr) and old (≳few Gyr) stellar populations. Using the Hδ equivalent widths we estimate that the burst masses must have been at least 10 per cent by mass ( M burst ≳ 10 10 M ⊙ ), which is also consistent with the star formation history inferred from the broad‐band spectral energy distributions. On average the A stars cover ∼33 per cent of the galaxy image, extending over 2–15 kpc 2 , indicating that the characteristic E+A signature is a property of the galaxy as a whole and not due to a heterogeneous mixture of populations. In approximately half of the sample, we find that the A stars, nebular emission and continuum emission are not co‐located, suggesting that the newest stars are forming in a different place than those that formed ≲1 Gyr ago, and that recent star formation has occurred in regions distinct from the oldest stellar populations. At least 10 of the galaxies (91 per cent) have dynamics that class them as ‘fast rotators’ with magnitudes, v /σ, λ R and bulge‐to‐total (B/T) ratio comparable to local, representative ellipticals and S0s. We also find a correlation between the spatial extent of the A stars and the dynamical state of the galaxy such that the fastest rotators tend to have the most compact A star populations, providing new constraints on models that aim to explain the transformation of later type galaxies into early types. Finally, we show that there are no obvious differences between the line extents and kinematics of E+A galaxies detected in the radio (active galactic nucleus, AGN) compared to non‐radio sources, suggesting that AGN feedback does not play a dramatic role in defining their properties, and/or that its effects are short.Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/90164/1/j.1365-2966.2011.20082.x.pd
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