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HOLY TRINITY CATHOLIC CHURCH CHIPPING NORTON 1836 - 20O8 to the Reader
HOLY TRINITY CATHOLIC CHURCH CHIPPING NORTON 1836 - 20O8 To The Reader. To-day, as we worship at Holy Trinity, we probably give few thoughts as to how there came to be a church here in the first place nor that, little more than one hundred and seventy years ago, life was not very easy as a practising Roman Catholic. Much of what we have today is due to three major physical influences down the years, the Earls of Shrewsbury (the Talbot family), the Jesuit Fathers and all those Religious who have served the Parish down the years. They all deserve our thanks and prayers. This rather leaves out the parishioners, but whether we like it or not, in real terms our role is a minor one even if for some it involves a lot of “minor work”. It might be better if more of us took more part in Parish affairs and spread the work load a bit but nevertheless, we should not overlook the role the Faith of parishioners has played in our small church, in the past and will continue to play into the future. This history is intended as a reminder of both the past and present parish and is concerned with three things – the physical structure of the church buildings, the Religious who have served the par- ish down the years and the parishioners for whom the Church and they exist. The origins of this and a Short History published earlier would not have come about without the suggestion of Father Frank Hull in 2006 and the major sources are acknowledged later. -
Oligarchs, King and Local Society: Medieval Slavonia
Antun Nekić OLIGARCHS, KING AND LOCAL SOCIETY: MEDIEVAL SLAVONIA 1301-1343 MA Thesis in Medieval Studies Central European University CEU eTD Collection Budapest May2015 OLIGARCHS, KING AND LOCAL SOCIETY: MEDIEVAL SLAVONIA 1301-1343 by Antun Nekić (Croatia) Thesis submitted to the Department of Medieval Studies, Central European University, Budapest, in partial fulfillment of the requirements of the Master of Arts degree in Medieval Studies. Accepted in conformance with the standards of the CEU. ____________________________________________ Chair, Examination Committee ____________________________________________ Thesis Supervisor ____________________________________________ Examiner CEU eTD Collection ____________________________________________ Examiner Budapest Month YYYY OLIGARCHS, KING AND LOCAL SOCIETY: MEDIEVAL SLAVONIA 1301-1343 by Antun Nekić (Croatia) Thesis submitted to the Department of Medieval Studies, Central European University, Budapest, in partial fulfillment of the requirements of the Master of Arts degree in Medieval Studies. Accepted in conformance with the standards of the CEU. CEU eTD Collection ____________________________________________ External Reader Budapest Month YYYY OLIGARCHS, KING AND LOCAL SOCIETY: MEDIEVAL SLAVONIA 1301-1343 by Antun Nekić (Croatia) Thesis submitted to the Department of Medieval Studies, Central European University, Budapest, in partial fulfillment of the requirements of the Master of Arts degree in Medieval Studies. Accepted in conformance with the standards of the CEU. ____________________________________________ External Supervisor CEU eTD Collection Budapest Month YYYY I, the undersigned, Antun Nekić, candidate for the MA degree in Medieval Studies, declare herewith that the present thesis is exclusively my own work, based on my research and only such external information as properly credited in notes and bibliography. I declare that no unidentified and illegitimate use was made of the work of others, and no part of the thesis infringes on any person’s or institution’s copyright. -
Viking Voice
- Winter 2 Fall - Winter 2018 Viking Voice A magazine for Lyndon Institute alumni, parents, and friends Project Bike Tech Comes to Lyndon Institute Head of School Twiladawn W. Perry ‘77 Letter from the Head of School.................. 1 Assistant Head for Curriculum & Instruction On Campus................................................4 Adam Norwood Chief Financial Officer Development...........................................10 Meagan N. Howard ‘02 Assistant Head for Student Experience Faculty and Staff..................................... 12 Robert G. Heath Jr. ‘88 President Project Bike Tech.................................... 14 Lawrence V. Cipollone Vice President Meredith R. Feltus ‘87 Athletics.................................................. 16 Secretary Nathan P. Sicard ‘00 Annual Giving......................................... 19 Tresurer David R. Hartwell ‘70 Alumni Weekend.................................... 28 Trustee At Large David R. Stahler, Sr. ‘65 Trustee At Large Class Reunions...................................... 31 David J. Beattie ‘61 Class Notes............................................ 34 Laurie Boswell Marlin W. Devenger ‘67 Patricia B. Emery ‘70 Commencement..................................... 40 Larissa Flynn T. Michael Flynn In Memoriam........................................... 43 Bretton J. Gale ‘77 James C. Gallagher ‘63 Daniel D. Heath ‘68 Spirit Week......................... Back Cover Peter C. Hopkins ‘74 Lorraine B. Impey ‘66 Noah N. Manning ‘13 Stephen Maleski Lorraine C. Matteis ‘65 Dr. Gregory -
23 Minor Planet Bulletin 41
23 observation interval. The overall form of the lightcurve did not of the other observatories. To make the large number of data points change perceptibly with phase angle or viewing aspect. in the segments of the lightcurve included by Organ Mesa observations more legible, those data have been binned in sets of Further evidence against the double period near 72.6 hours is five points with a maximum of ten minutes between points. provided by Schober et al. (1993). They draw a composite bimodal lightcurve phased to 36.0 hours based on data from 6 consecutive References nights with about 60% phase coverage. Overlapping sessions on this lightcurve centered near 1989 Nov 30.3 and Dec 3.3 each Behrend, R. (2005). Observatoire de Geneve web site. show a small rise followed by a fall greater than 0.4 magnitudes in http://obswww.unige.ch/~behrend/page_cou.html about 6 hours. This sets a lower limit in their data for the amplitude. An amplitude as large as 0.4 magnitudes is possible Higgins, D.J., Menke, J., Pozzoli, V., Sheridan, E., and Dymock, only for a bimodal lightcurve. R. (2004). “Lightcurve and Period Determination for 582 Olympia.” Minor Planet Bull. 31, 12. Independently, Franco drew an H-G plot based only on sparse data from the U.S. Naval Observatory (USNO), i.e., not including any JPL (2013). http://ssd.jpl.nasa.gov/sbdb.cgi of the new photometry. These data contain no correction for rotational variation and in include the inherent scatter in the USNO Menke, J. (2011). Menke Scientific, Ltd. -
The Warped Ways of Cosmic Light
BIOLOGIE & MEDIZIN_Infektionsbiologie “Around that area there are indeed numerous small nebulous patches so close together that, upon seeing the region, one is positively startled by the strange appearance of this ‘nebula cluster’.” This was the sentiment expressed by Heidelberg-based astronomer Max Wolf in 1901 about the galaxy cluster in the constellation Coma Berenices. The cluster Abell 2218 presents a similar appearance to the viewer today on this image from the Hubble Space Telescope. The “strange appearance” – the many blue and orange arcs – owes, in this case, to the effect of a gravitational lens. PHYSICS & ASTRONOMY_Gravitational Lenses The Warped Ways of Cosmic Light Albert Einstein predicted them, modern giant telescopes detected them – and Klaus Dolag simulates them on a computer: gravitational lenses. The academic staff member at the Max Planck Institute for Astrophysics in Garching and at the University Observatory Munich uses this physical phenomenon to such ends as weighing galaxy clusters and probing that ominous substance known as dark matter. TEXT HELMUT HORNUNG he sky over Principe was a total eclipse of the Sun. The test was More recent analyses of Eddington’s cloudy and the mood in the simple: if a massive object bends space, findings show that the values measured camp on the coconut plan- then the Sun must also cause the pass- at that time did, indeed, correspond to tation had hit rock bottom. ing light from stars to deviate from its the prediction, but that they are appar- Having set out from Eng- straight course. In other words, the ently the result of an instrument error T land, the men had been traveling for points of light in the immediate vicin- of, as it so happens, the very same mag- weeks to reach the volcanic island in ity of the black Sun should be shifted nitude. -
Trojan Search at ESO E
Lf) provide an effective method (a) to dis Kron and A Renzini, (Dordrecht: Reidel), o criminate galaxy morphology, (b) to p.61. evaluate their intrinsic evolution and (c) Buzzoni, A: 1988, in preparation. Butcher, H. and Oemler, A.: 1984, Ap. J., 285, to estimate redshift with an accuracy of 426. 0.05. We emphasize that two main ± Coleman, G.D., Wu, C. C. and Weedman, ...--...0 requirements have to be fulfilled in order Q() D. W.: 1980, Ap. J. Supp., 43, 393. <\l to reach such a fair resolution in explor Couch, W.J. and Newell, E. B.: 1984, Ap. J., E ing the universe at large distances: 56,143. '-' <J Lf) (i) we need to observe clusters instead Couch, W.J., Ellis, R.S., Godwin, J. and Car o o of field galaxies to be able to recognize ter, 0.: 1983, MN.R.A.S., 205,1287. them with high statistical confidence; Ellis, R. S., Couch, W. J., Maclaren, I. and (ii) we need a combined comparison Koo, D.C.: 1985, MN.R.A.S., 217, 239. 2158+0351 Gunn, J. E., Hoessel, I. G. and Oke, J. B.: with evolutionary models, in order to 1986, Ap. J., 306, 30. properly account for the intrinsic photo Koo, D. C.: 1981, Ap. J. (Lett), 251, L 75. 0.4 0.5 metric properties as we use galaxies as Loh, E.D. and Spillar, E.J.: 1986, Ap. J., 303, REDSHI8 T standard candles in the cosmological 154. Figure 8: The photometrie determination of framework. Maclaren, 1., Ellis, R.S. and Couch, W.J.: the redshift of the cluster 2158 + 0351. -
The Ginger Fox's Two Crowns Central Administration and Government in Sigismund of Luxembourg's Realms
Doctoral Dissertation THE GINGER FOX’S TWO CROWNS CENTRAL ADMINISTRATION AND GOVERNMENT IN SIGISMUND OF LUXEMBOURG’S REALMS 1410–1419 By Márta Kondor Supervisor: Katalin Szende Submitted to the Medieval Studies Department, Central European University, Budapest in partial fulfillment of the requirements for the degree of Doctor of Philosophy in Medieval Studies, CEU eTD Collection Budapest 2017 Table of Contents I. INTRODUCTION 6 I.1. Sigismund and His First Crowns in a Historical Perspective 6 I.1.1. Historiography and Present State of Research 6 I.1.2. Research Questions and Methodology 13 I.2. The Luxembourg Lion and its Share in Late-Medieval Europe (A Historical Introduction) 16 I.2.1. The Luxembourg Dynasty and East-Central-Europe 16 I.2.2. Sigismund’s Election as King of the Romans in 1410/1411 21 II. THE PERSONAL UNION IN CHARTERS 28 II.1. One King – One Land: Chancery Practice in the Kingdom of Hungary 28 II.2. Wearing Two Crowns: the First Years (1411–1414) 33 II.2.1. New Phenomena in the Hungarian Chancery Practice after 1411 33 II.2.1.1. Rex Romanorum: New Title, New Seal 33 II.2.1.2. Imperial Issues – Non-Imperial Chanceries 42 II.2.2. Beginnings of Sigismund’s Imperial Chancery 46 III. THE ADMINISTRATION: MOBILE AND RESIDENT 59 III.1. The Actors 62 III.1.1. At the Travelling King’s Court 62 III.1.1.1. High Dignitaries at the Travelling Court 63 III.1.1.1.1. Hungarian Notables 63 III.1.1.1.2. Imperial Court Dignitaries and the Imperial Elite 68 III.1.1.2. -
Monastic Landscapes of Medieval Transylvania (Between the Eleventh and Sixteenth Centuries)
DOI: 10.14754/CEU.2020.02 Doctoral Dissertation ON THE BORDER: MONASTIC LANDSCAPES OF MEDIEVAL TRANSYLVANIA (BETWEEN THE ELEVENTH AND SIXTEENTH CENTURIES) By: Ünige Bencze Supervisor(s): József Laszlovszky Katalin Szende Submitted to the Medieval Studies Department, and the Doctoral School of History Central European University, Budapest of in partial fulfillment of the requirements for the degree of Doctor of Philosophy in Medieval Studies, and CEU eTD Collection for the degree of Doctor of Philosophy in History Budapest, Hungary 2020 DOI: 10.14754/CEU.2020.02 ACKNOWLEDGMENTS My interest for the subject of monastic landscapes arose when studying for my master’s degree at the department of Medieval Studies at CEU. Back then I was interested in material culture, focusing on late medieval tableware and import pottery in Transylvania. Arriving to CEU and having the opportunity to work with József Laszlovszky opened up new research possibilities and my interest in the field of landscape archaeology. First of all, I am thankful for the constant advice and support of my supervisors, Professors József Laszlovszky and Katalin Szende whose patience and constructive comments helped enormously in my research. I would like to acknowledge the support of my friends and colleagues at the CEU Medieval Studies Department with whom I could always discuss issues of monasticism or landscape archaeology László Ferenczi, Zsuzsa Pető, Kyra Lyublyanovics, and Karen Stark. I thank the director of the Mureş County Museum, Zoltán Soós for his understanding and support while writing the dissertation as well as my colleagues Zalán Györfi, Keve László, and Szilamér Pánczél for providing help when I needed it. -
The Internal Structure of the Asteroids
**FULL TITLE** ASP Conference Series, Vol. **VOLUME**, **YEAR OF PUBLICATION** **NAMES OF EDITORS** The internal structure of the asteroids V.Celebonovi´cˇ Inst.of Physics,Pregrevica 118,11080 Zemun-Beograd,Serbia Abstract. Knowledge of the internal structure of the asteroids is rather poorly developed,mainly due to lack of reliable data (masses or densities and radii). This contribution has two aims: to review the basics of existing knowledge and explore the possibility of advancing the field by introducing and using in it some well known ideas from solid state physics. 1. Introduction The largest part of astronomical research directly relies on data taken at various kinds of telescopes of variable size - from those having mirrors of 8 or 10 meters in diameter to backyard amateur telescopes. However,serious comlications arise when one attempts to gain information on the internal structure of any kind of celestial bodies. The reason for these complications is simple: the interiors of any kind of objects are unobservable. For example, nobody has ever gone (and nobody ever will) into the center of Jupiter to measure the temperature there. Surfaces of many kinds of objects are observable. However, the ”state” of a surface of any given object is a consequence of at least two factors: processes occuring in the interior of the object but also of any possible external influences. The aim of this lecture is to discuss to some extent one particular ”subfield” within the field of modelling of the internal structure of celestial objects - the internal structure of the asteroids. Apart from the introduction,this contribution has three more parts. -
Frank Schlesinger 1871-1943
NATIONAL ACADEMY OF SCIENCES OF THE UNITED STATES OF AMERICA BIOGRAPHICAL MEMOIRS VOLUME XXIV THIRD MEMOIR BIOGRAPHICAL MEMOIR OF FRANK SCHLESINGER 1871-1943 BY DIRK BROUWER PRESENTED TO THE ACADEMY AT THE ANNUAL MEETING, 1945 FRANK SCHLESINGER 1871-1943 BY DIRK BROUWER Frank Schlesinger was born in New York City on May n, 1871. His father, William Joseph Schlesinger (1836-1880), and his mother, Mary Wagner Schlesinger (1832-1892), both natives of the German province of Silesia, had emigrated to the United States. In Silesia they had lived in neighboring vil- lages, but they did not know each other until they met in New York, in 1855, at the home of Mary's cousin. They were mar- ried in 1857 and had seven children, all of whom grew to maturity. Frank was the youngest and, after 1939, the last survivor. His father's death, in 1880, although it brought hardships to the family, was not permitted to interfere with Frank's educa- tion. He attended public school in New York City, and eventually entered the College of the City of New York, receiv- ing the degree of Bachelor of Science in 1890. His aptitude for mathematical science, already evident in grammar school, be- came more marked in the higher stages of his education when he began to show a preference for applied mathematics. Upon completing his undergraduate work it was not possible for him to continue with graduate studies. He had to support himself, and his health at that time made it desirable for him to engage in outdoor activities. -
Harold Knox-Shaw and the Helwan Observatory
1 Harold Knox-Shaw and the Helwan Observatory Jeremy Shears & Ashraf Ahmed Shaker Abstract Harold Knox-Shaw (1885-1970) worked at the Helwan Observatory in Egypt from 1907 to 1924. The Observatory was equipped with a 30-inch (76 cm) reflector that was financed and constructed by the Birmingham industrialist, John Reynolds (1874- 1949), to benefit from the clearer skies and more southerly latitude compared with Britain. Knox-Shaw obtained the first photograph of Halley’s Comet on its 1910 perihelion passage. He also carried out morphological studies on nebulae and may have been the first to identify what later became to be known as elliptical galaxies as a distinct class of object. Photographic analysis of the variable nebula NGC 6729 in Corona Australis enabled him to conclude that the changes in brightness and shape were correlated with the light travel time from the illuminating star, R CrA. Introduction By the beginning of the twentieth century fundamental changes in astronomy were well-advanced, with a move from a traditional positional and descriptive approach to the new science of astrophysics. This was driven by the development of two new tools: spectroscopy and photography. In Great Britain the chief practitioners of the science were no longer the self-taught individuals of independent wealth, the Grand Amateurs of the Victorian age, but increasingly they were University-trained scientists employed by professional research institutions (1). Across the Atlantic, the United States was making great strides in the development of the new astronomy. Here, in the first two decades of the twentieth century increasingly large telescopes were being built to generate astrophysical data, such as the giant reflectors on Mount Wilson which benefitted from the clear skies and southerly latitudes of California. -
Roman Catholic Church Case Study: Archdiocese of Birmingham
The Roman Catholic Church Case Study: Archdiocese of Birmingham Investigation Report June 2019 2019 The Roman Catholic Church Case Study: Archdiocese of Birmingham Investigation Report June 2019 A report of the Inquiry Panel Professor Alexis Jay OBE Professor Sir Malcolm Evans KCMG OBE Ivor Frank Drusilla Sharpling CBE © Crown copyright 2019 The text of this document (this excludes, where present, the Royal Arms and all departmental or agency logos) may be reproduced free of charge in any format or medium provided that it is reproduced accurately and not in a misleading context. The material must be acknowledged as Crown copyright and the document title specified. Where third‑party material has been identified, permission from the respective copyright holder must be sought. Any enquiries related to this publication should be sent to us at [email protected] or Freepost IICSA INDEPENDENT INQUIRY. This publication is available at https://www.iicsa.org.uk/reports CCS0519276634 06/19 Printed on paper containing 75% recycled‑fibre content minimum. Printed in the UK by the APS Group on behalf of the Controller of Her Majesty’s Stationery Office. The following corrections were made to the report on 23 July 2019: Page 17: clarification of language – ‘anally rape’ changed to ‘sexually abuse’. Contents Executive Summary i Part A: Introduction 1 A.1: The background to the investigation 2 A.2: Scope of the investigation 3 A.3: Procedure adopted by the Inquiry 4 A.4: Terminology 5 Part B: The Archdiocese of Birmingham 7 B.1: The structure of the