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La Constellation Du Taureau
La constellation du Taureau La constellation zodiacale du Taurus – le Taureau – est parfaitement visible sous les deux hémisphères d’avril à février. (1) Un peu de mythologie Selon la légende, l’œil rouge du puissant Taureau surveille Orion, le Chasseur, des avances duquel il veut protéger les Sept Sœurs – les Pléiades -. Le cœur d’Orion est tourné vers Mérope, l’une des sœurs dont il veut faire sa femme cependant qu’au bord de l’Amas des Pléiades, les parents de celle-ci le Titan Atlas et l’Océanide Pléioné – les observent attentivement. Des sept Pléiades, jeunes étoiles bleues saphir, seule Mérope a épousé un mortel, le roi de Corinthe, aussi cache-t-elle sa honte derrière une fine nébuleuse par réflexion. (2) (1) et (2) L’exploration du ciel, Robert Burnham, Alan Dyer, Robert A. Garfinkle, Martin George, Jeff Kanipi, David H. Levy. Édition Konemann, page 202. Chez les Babyloniens, le fermier (maintenant le Bélier) guide un Taureau qui manœuvre une charrue céleste creusant un sillon dans le ciel le long de l’écliptique. (3) Les Hyades sont les filles du dieu Atlas et de Pléione. Elles étaient 15 et avaient un frère nommé Hyas. Quand Hyas fut tué par un lion cinq des filles étaient inconsolables et ont été mises dans le ciel près de Hyas (constellation du Verseau) et ont été appelées les Hyades pour faire honneur à leur frère. Les sœurs qui restèrent pleuraient celles qui avaient été placées dans le ciel et à leur tour, s’y retrouvèrent et sont devenues les Pléiades. (4) (3) et (4) L’Observateur, revue électronique, http://astrosurf.com/duplessis/observateur/revue.html Volume 3, numéro 3, Constellation et ses étoiles, Rachelle Léger de la SAPM, page 2 Les Hyades (Mel 25) et les Pléiades (M 45) sont deux objets du ciel profond apparaissant dans le catalogue d’observation du CAABM. -
From Bats to Weta Holy Grail of Educational Research a Word From
October 2013 | Faculty of Science Alumni Magazine Issue 07 Clearing the air in Auckland How coffee can benefit your job Iconic species – from bats to weta Holy Grail of educational research A word from The University of Auckland Faculty of Science alumni magazine the Dean 2013 Editorial team: New Zealand has always had an impressive reputation for Rebekah Holmes, Linda Thompson innovation, and there’s growing awareness that science and Feature writer: Pauline Curtis innovation are critical to our future economic success. News writers: You can also read about how our mathematics Sabine Kruekel, Judith Poland department is keeping us at the forefront of Design: Timberlake Studio Ltd research and innovation in tertiary education. We’re very proud of the quality of teaching in Faculty of Science the Faculty. Our researchers’ success in their bid for this project, and the 2013 national Email: [email protected] teaching excellence award to Associate www.science.auckland.ac.nz/inscight Professor Cather Simpson, are just two examples of this. How alumni keep in touch Congratulations too, to the many other staff, Professor Grant Guilford, Dean of Science To ensure that you continue to receive students and alumni who have won accolades InSCight, and to subscribe to @Auckland, In recent years the Faculty of Science has this year, from honours for lifetime the University’s email newsletter for alumni achievement like Distinguished Professor and friends, please update your details: developed a comprehensive suite of initiatives to support key sectors of the New Zealand Margaret Brimble’s Rutherford Medal, Email: [email protected] economy, from the dairy industry to Professor James Goodman’s Eckert-Mauchly www.alumni.auckland.ac.nz/update biotechnology and high-tech manufacturing. -
Observations of T-Tauri Stars Using HST-GHRS: II. Optical and Near UV Lines David R
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by CERN Document Server Submitted to ApJ Observations of T-Tauri Stars using HST-GHRS: II. Optical and Near UV lines David R. Ardila1, Gibor Basri2, Frederick M. Walter3, Jeff A. Valenti4, Christopher M. Johns-Krull5 ABSTRACT We have analyzed GHRS data of eight Classical T Tauri stars (CTTSs) and one Weak T Tauri star (WTTS). The GHRS data consist of an spectral range 40 A˚ wide centered on 2800 A.˚ For 4 of the CTTS we have nearly simultaneous optical observations which contain Hα,Hβ,HeI,NaD,andtheCaII infrared triplet. The Mg II resonance doublet is the strongest feature in the 2800 A˚ range. This line has a fairly wide and symmetric emission component ( 200 1 ∼ to 300 km s− for the CTTSs), with a narrow central absorption and a wide ∼ blueshifted absorption superimposed to it. The narrow central absorption width and equivalent width are inconsistent with being due only to ISM clouds described in the literature, which lead us to conclude that it is partially due to non-LTE processes in the emission line region itself. The emission profile closely follows Hα. Its large width in CTTS cannot be due to the Stark effect and we suggest that it is due to supersonic turbulence. All the stars show blueshifted absorptions 1 that are evidence of outflows (terminal velocities 300 km s− ), with multiple ∼ flows observed in two stars. We show evidence that the wind is not spherical, with wind signatures being stronger for lower inclinations at a given accretion rate. -
Variable Star Section Circular
British Astronomical Association Variable Star Section Circular No 82, December 1994 CONTENTS A New Director 1 Credit for Observations 1 Submission of 1994 Observations 1 Chart Problems 1 Recent Novae Named 1 Z Ursae Minoris - A New R CrB Star? 2 The February 1995 Eclipse of 0¼ Geminorum 2 Computerisation News - Dave McAdam 3 'Stella Haitland, or Love and the Stars' - Philip Hurst 4 The 1994 Outburst of UZ Bootis - Gary Poyner 5 Observations of Betelgeuse by the SPA-VSS - Tony Markham 6 The AAVSO and the Contribution of Amateurs to VS Research Suspected Variables - Colin Henshaw 8 From the Literature 9 Eclipsing Binary Predictions 11 Summaries of IBVS's Nos 4040 to 4092 14 The BAA Instruments and Imaging Section Newsletter 16 Light-curves (TZ Per, R CrB, SV Sge, SU Tau, AC Her) - Dave McAdam 17 ISSN 0267-9272 Office: Burlington House, Piccadilly, London, W1V 9AG Section Officers Director Tristram Brelstaff, 3 Malvern Court, Addington Road, READING, Berks, RG1 5PL Tel: 0734-268981 Section Melvyn D Taylor, 17 Cross Lane, WAKEFIELD, Secretary West Yorks, WF2 8DA Tel: 0924-374651 Chart John Toone, Hillside View, 17 Ashdale Road, Cressage, Secretary SHREWSBURY, SY5 6DT Tel: 0952-510794 Computer Dave McAdam, 33 Wrekin View, Madeley, TELFORD, Secretary Shropshire, TF7 5HZ Tel: 0952-432048 E-mail: COMPUSERV 73671,3205 Nova/Supernova Guy M Hurst, 16 Westminster Close, Kempshott Rise, Secretary BASINGSTOKE, Hants, RG22 4PP Tel & Fax: 0256-471074 E-mail: [email protected] [email protected] Pro-Am Liaison Roger D Pickard, 28 Appletons, HADLOW, Kent TN11 0DT Committee Tel: 0732-850663 Secretary E-mail: [email protected] KENVAD::RDP Eclipsing Binary See Director Secretary Circulars Editor See Director Telephone Alert Numbers Nova and First phone Nova/Supernova Secretary. -
Des Projets D'envergure Astro Débutant Ciel Profond
Une publication de la Société d’astronomie du Planétarium de Montréal • SAPM Hiver 2014-2015 — volume 25, numéro 4 Le ciel des Hommes par Gilbert St-Onge - p.4 Des projets d’envergure par Gilbert St-Onge - p.8 Astro débutant par Charles Gagné - p.10 Ciel profond par Suzanne Parent - p.14 Photos : Sarah Cartwright, Gilbert Cartwright, : Sarah Photos et HST St-Onge CONVENTION DE LA POSTE-PUBLICATIONS No 41017003 Retourner toute correspondance ne pouvant être livrée Mot du Président - Malgré le froid, profitez du ciel de l’hiver au Canada au Service des publications 123, rue Sainte-Catherine, Montréal, QC, H3Z 2Y7 Courriel : [email protected] Les belles soirées d’astronomie d’hiver sont à nos Société d’astronomie du Planétarium de Montréal portes. Nous pourrons profiter d’une durée de la nuit plus 4801, av. Pierre-de Coubertin, Montréal (QC) H1V 3V4 www.sapm.qc.ca longue et de ciels généralement plus cristallins, mais il faudra Facebook : facebook.com/ s’habiller chaudement. Societedastronomieduplanetariumdemontreal Twitter : twitter.com/sapm_astro La technique de l’oignon est la meilleure méthode pour pou- La Société d’astronomie du Planétarium de Montréal voir rester au chaud. Portez d’abord d’une première couche de (SAPM) est un organisme à but non lucratif dont les sous-vêtements chauds. Ajoutez ensuite une seconde plus épaisse principaux objectifs sont de promouvoir l’astronomie auprès du grand public en organisant des événements de type fibre polaire pour retenir la chaleur et terminez par une spéciaux lors de différents phénomènes astronomiques couche très chaude qui retiendra la chaleur et coupera le vent (pluies d’étoiles filantes, éclipses, comètes brillantes, etc.), de favoriser les échanges entre les astronomes amateurs glacial d’hiver. -
Information Bulletin on Variable Stars
COMMISSIONS AND OF THE I A U INFORMATION BULLETIN ON VARIABLE STARS Nos November July EDITORS L SZABADOS K OLAH TECHNICAL EDITOR A HOLL TYPESETTING K ORI ADMINISTRATION Zs KOVARI EDITORIAL BOARD L A BALONA M BREGER E BUDDING M deGROOT E GUINAN D S HALL P HARMANEC M JERZYKIEWICZ K C LEUNG M RODONO N N SAMUS J SMAK C STERKEN Chair H BUDAPEST XI I Box HUNGARY URL httpwwwkonkolyhuIBVSIBVShtml HU ISSN COPYRIGHT NOTICE IBVS is published on b ehalf of the th and nd Commissions of the IAU by the Konkoly Observatory Budap est Hungary Individual issues could b e downloaded for scientic and educational purp oses free of charge Bibliographic information of the recent issues could b e entered to indexing sys tems No IBVS issues may b e stored in a public retrieval system in any form or by any means electronic or otherwise without the prior written p ermission of the publishers Prior written p ermission of the publishers is required for entering IBVS issues to an electronic indexing or bibliographic system to o CONTENTS C STERKEN A JONES B VOS I ZEGELAAR AM van GENDEREN M de GROOT On the Cyclicity of the S Dor Phases in AG Carinae ::::::::::::::::::::::::::::::::::::::::::::::::::: : J BOROVICKA L SAROUNOVA The Period and Lightcurve of NSV ::::::::::::::::::::::::::::::::::::::::::::::::::: :::::::::::::: W LILLER AF JONES A New Very Long Period Variable Star in Norma ::::::::::::::::::::::::::::::::::::::::::::::::::: :::::::::::::::: EA KARITSKAYA VP GORANSKIJ Unusual Fading of V Cygni Cyg X in Early November ::::::::::::::::::::::::::::::::::::::: -
2010 Academy Annual Report
This document has been created from historical website content. 2010 Academy Annual Report The 2010 Academy Annual Report details the accomplishments of the Academy of the Royal Society of New Zealand throughout the year. Chair’s foreword In January 2010 the final act of “embracing the Humanities” within the Royal Society took place with the signing of an MOU between Te Whainga Aronui The Council for the Humanities and Te Apārangi the Royal Society of New Zealand. President Dr Garth Carnaby described this as landmark decision for both organisations. “For the first time there will be an organisation in New Zealand that promotes excellence in research and scholarship across all the disciplines and areas of knowledge.” The CV’s of the existing fellows of the Council for the Humanities were reviewed by the Academy Executive and these people were admitted to the Fellowship by a special resolution at the Fellow’s AGM. The Academy has continued to provide “information pieces” and forward- looking contributions on present and emerging debates that were introduced in 2009. In 2010, 2 information statements were prepared. Sea Level Rise: Emerging Issues recounted the significant changes in the scientific understanding of this issue since the 2007 Assessment Report by the IPCC. The Darfield Earthquake: The Value of Long-term Research was produced to document the research conducted in New Zealand over many years on how to construct and strengthen buildings to improve performance during large earthquakes. The application of this science and engineering undoubtedly played a big role in limiting the damage and injury caused by the 2010 Christchurch earthquake. -
The Philosophy of Cosmology Edited by Khalil Chamcham , Joseph Silk , John D
Cambridge University Press 978-1-107-14539-9 — The Philosophy of Cosmology Edited by Khalil Chamcham , Joseph Silk , John D. Barrow , Simon Saunders Frontmatter More Information THE PHILOSOPHY OF COSMOLOGY Following a long-term international collaboration between leaders in cosmology and the philosophy of science, this volume addresses foundational questions at the limits of sci- ence across these disciplines, questions raised by observational and theoretical progress in modern cosmology. Space missions have mapped the Universe up to its early instants, opening up questions on what came before the Big Bang, the nature of space and time, and the quantum origin of the Universe. As the foundational volume of an emerging academic discipline, experts from relevant fields lay out the fundamental problems of contemporary cosmology and explore the routes toward possible solutions. Written for physicists and philosophers, the emphasis is on con- ceptual questions, and on ways of framing them that are accessible to each community and to a still wider readership: those who wish to understand our modern vision of the Universe, its unavoidable philosophical questions, and its ramifications for scientific methodology. KHALIL CHAMCHAM is a researcher at the University of Oxford. He acted as the exec- utive director of the UK collaboration on the ‘Philosophy of Cosmology’ programme. His main research interests are in the chemical evolution of galaxies, nucleosynthesis, dark matter, and the concept of time. He has co-authored four books and co-edited ten, includ- ing From Quantum Fluctuations to Cosmological Structures and Science and Search for Meaning. JOSEPH SILK FRS is Homewood Professor at the Johns Hopkins University, Research Scientist at the Institut d’Astrophysique de Paris, CNRS and Sorbonne Universities, and Senior Fellow at the Beecroft Institute for Particle Astrophysics at the University of Oxford. -
Religion in an Age of Science by Ian Barbour
Religion in an Age of Science return to religion-online 47 Religion in an Age of Science by Ian Barbour Ian G. Barbour is Professor of Science, Technology, and Society at Carleton College, Northefiled, Minnesota. He is the author of Myths, Models and Paradigms (a National Book Award), Issues in Science and Religion, and Science and Secularity, all published by HarperSanFrancisco. Published by Harper San Francisco, 1990. This material was prepared for Religion Online by Ted and Winnie Brock. (ENTIRE BOOK) An excellent and readable summary of the role of religion in an age of science. Barbour's Gifford Lectures -- the expression of a lifetime of scholarship and deep personal conviction and insight -- including a clear and helpful analysis of process theology. Preface What is the place of religion in an age of science? How can one believe in God today? What view of God is consistent with the scientific understanding of the world? My goals are to explore the place of religion in an age of science and to present an interpretation of Christianity that is responsive to both the historical tradition and contemporary science. Part 1: Religion and the Methods of Science Chapter 1: Ways of Relating Science and Religion A broad description of contemporary views of the relationship between the methods of science and those of religion: Conflict, Independence, Dialogue, and Integration. Chapter 2: Models and Paradigms This chapter examines some parallels between the methods of science and those of religion: the interaction of data and theory (or experience and interpretation); the historical character of the interpretive community; the use of models; and the influence of paradigms or programs. -
COMMISSIONS 27 and 42 of the I.A.U. INFORMATION BULLETIN on VARIABLE STARS Nos. 4101{4200 1994 October { 1995 May EDITORS: L. SZ
COMMISSIONS AND OF THE IAU INFORMATION BULLETIN ON VARIABLE STARS Nos Octob er May EDITORS L SZABADOS and K OLAH TECHNICAL EDITOR A HOLL TYPESETTING K ORI KONKOLY OBSERVATORY H BUDAPEST PO Box HUNGARY IBVSogyallakonkolyhu URL httpwwwkonkolyhuIBVSIBVShtml HU ISSN 2 CONTENTS 1994 No page E F GUINAN J J MARSHALL F P MALONEY A New Apsidal Motion Determination For DI Herculis ::::::::::::::::::::::::::::::::::::: D TERRELL D H KAISER D B WILLIAMS A Photometric Campaign on OW Geminorum :::::::::::::::::::::::::::::::::::::::::::: B GUROL Photo electric Photometry of OO Aql :::::::::::::::::::::::: LIU QUINGYAO GU SHENGHONG YANG YULAN WANG BI New Photo electric Light Curves of BL Eridani :::::::::::::::::::::::::::::::::: S Yu MELNIKOV V S SHEVCHENKO K N GRANKIN Eclipsing Binary V CygS Former InsaType Variable :::::::::::::::::::: J A BELMONTE E MICHEL M ALVAREZ S Y JIANG Is Praesep e KW Actually a Delta Scuti Star ::::::::::::::::::::::::::::: V L TOTH Ch M WALMSLEY Water Masers in L :::::::::::::: R L HAWKINS K F DOWNEY Times of Minimum Light for Four Eclipsing of Four Binary Systems :::::::::::::::::::::::::::::::::::::::::: B GUROL S SELAN Photo electric Photometry of the ShortPeriod Eclipsing Binary HW Virginis :::::::::::::::::::::::::::::::::::::::::::::: M P SCHEIBLE E F GUINAN The Sp otted Young Sun HD EK Dra ::::::::::::::::::::::::::::::::::::::::::::::::::: ::::::::::::: M BOS Photo electric Observations of AB Doradus ::::::::::::::::::::: YULIAN GUO A New VR Cyclic Change of H in Tau :::::::::::::: -
Research and Scientific Support Department 2003 – 2004
COVER 7/11/05 4:55 PM Page 1 SP-1288 SP-1288 Research and Scientific Research Report on the activities of the Support Department Research and Scientific Support Department 2003 – 2004 Contact: ESA Publications Division c/o ESTEC, PO Box 299, 2200 AG Noordwijk, The Netherlands Tel. (31) 71 565 3400 - Fax (31) 71 565 5433 Sec1.qxd 7/11/05 5:09 PM Page 1 SP-1288 June 2005 Report on the activities of the Research and Scientific Support Department 2003 – 2004 Scientific Editor A. Gimenez Sec1.qxd 7/11/05 5:09 PM Page 2 2 ESA SP-1288 Report on the Activities of the Research and Scientific Support Department from 2003 to 2004 ISBN 92-9092-963-4 ISSN 0379-6566 Scientific Editor A. Gimenez Editor A. Wilson Published and distributed by ESA Publications Division Copyright © 2005 European Space Agency Price €30 Sec1.qxd 7/11/05 5:09 PM Page 3 3 CONTENTS 1. Introduction 5 4. Other Activities 95 1.1 Report Overview 5 4.1 Symposia and Workshops organised 95 by RSSD 1.2 The Role, Structure and Staffing of RSSD 5 and SCI-A 4.2 ESA Technology Programmes 101 1.3 Department Outlook 8 4.3 Coordination and Other Supporting 102 Activities 2. Research Activities 11 Annex 1: Manpower Deployment 107 2.1 Introduction 13 2.2 High-Energy Astrophysics 14 Annex 2: Publications 113 (separated into refereed and 2.3 Optical/UV Astrophysics 19 non-refereed literature) 2.4 Infrared/Sub-millimetre Astrophysics 22 2.5 Solar Physics 26 Annex 3: Seminars and Colloquia 149 2.6 Heliospheric Physics/Space Plasma Studies 31 2.7 Comparative Planetology and Astrobiology 35 Annex 4: Acronyms 153 2.8 Minor Bodies 39 2.9 Fundamental Physics 43 2.10 Research Activities in SCI-A 45 3. -
How Special Is Our Universe? Fine-Tuning and Cosmological Natural Selection
6 DECEMBER 2017 How Special is our Universe? Fine-Tuning and Cosmological Natural Selection PROFESSOR JOSEPH SILK Fine-tuning in Nature If the fundamental constants of nature differed from their measured values, life as we know it would not have emerged. Imagine a universe in which the fine structure constant was slightly larger or smaller than the actual value that we measure. Stars like the sun are witness to a titanic battle between the forces of electromagnetism and gravity. The solar system formed from the ashes of burnt-out stars. Displace this equilibrium slightly and the very existence of nuclear-burning stars is at risk. In such a universe, stars would never have formed, or might have collapsed to black holes. Perhaps there are many other universes, most of which are uncongenial to life. Theories of the multiverse are designed to accommodate the possibility that there are only incredibly rare examples of life-containing universes. We live in one of these, whether by cosmological natural selection or by the consequences of an ultimate theory that has yet to be formulated. Simple physical arguments can account for the fundamental scaling relations of stars and galaxies. To be fair to simulators, the dispersion in these relations contains most of the relevant physics, and can only be adequately explored via state-of-the-art numerical simulations over a vast and currently inadequate dynamical range. Here however I focus here not on the scaling laws but on the actual scales: characteristic, minimum and maximum, from protostars to stars, galaxies and supermassive black holes. Unlike the scientists of antiquity, astronomers today have two significant advantages.