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Ira Sprague Bowen Papers, 1940-1973
http://oac.cdlib.org/findaid/ark:/13030/tf2p300278 No online items Inventory of the Ira Sprague Bowen Papers, 1940-1973 Processed by Ronald S. Brashear; machine-readable finding aid created by Gabriela A. Montoya Manuscripts Department The Huntington Library 1151 Oxford Road San Marino, California 91108 Phone: (626) 405-2203 Fax: (626) 449-5720 Email: [email protected] URL: http://www.huntington.org/huntingtonlibrary.aspx?id=554 © 1998 The Huntington Library. All rights reserved. Observatories of the Carnegie Institution of Washington Collection Inventory of the Ira Sprague 1 Bowen Papers, 1940-1973 Observatories of the Carnegie Institution of Washington Collection Inventory of the Ira Sprague Bowen Paper, 1940-1973 The Huntington Library San Marino, California Contact Information Manuscripts Department The Huntington Library 1151 Oxford Road San Marino, California 91108 Phone: (626) 405-2203 Fax: (626) 449-5720 Email: [email protected] URL: http://www.huntington.org/huntingtonlibrary.aspx?id=554 Processed by: Ronald S. Brashear Encoded by: Gabriela A. Montoya © 1998 The Huntington Library. All rights reserved. Descriptive Summary Title: Ira Sprague Bowen Papers, Date (inclusive): 1940-1973 Creator: Bowen, Ira Sprague Extent: Approximately 29,000 pieces in 88 boxes Repository: The Huntington Library San Marino, California 91108 Language: English. Provenance Placed on permanent deposit in the Huntington Library by the Observatories of the Carnegie Institution of Washington Collection. This was done in 1989 as part of a letter of agreement (dated November 5, 1987) between the Huntington and the Carnegie Observatories. The papers have yet to be officially accessioned. Cataloging of the papers was completed in 1989 prior to their transfer to the Huntington. -
A Propensity for Genius: That Something Special About Fritz Zwicky (1898 - 1974)
Swiss American Historical Society Review Volume 42 Number 1 Article 2 2-2006 A Propensity for Genius: That Something Special About Fritz Zwicky (1898 - 1974) John Charles Mannone Follow this and additional works at: https://scholarsarchive.byu.edu/sahs_review Part of the European History Commons, and the European Languages and Societies Commons Recommended Citation Mannone, John Charles (2006) "A Propensity for Genius: That Something Special About Fritz Zwicky (1898 - 1974)," Swiss American Historical Society Review: Vol. 42 : No. 1 , Article 2. Available at: https://scholarsarchive.byu.edu/sahs_review/vol42/iss1/2 This Article is brought to you for free and open access by BYU ScholarsArchive. It has been accepted for inclusion in Swiss American Historical Society Review by an authorized editor of BYU ScholarsArchive. For more information, please contact [email protected], [email protected]. Mannone: A Propensity for Genius A Propensity for Genius: That Something Special About Fritz Zwicky (1898 - 1974) by John Charles Mannone Preface It is difficult to write just a few words about a man who was so great. It is even more difficult to try to capture the nuances of his character, including his propensity for genius as well as his eccentric behavior edging the abrasive as much as the funny, the scope of his contributions, the size of his heart, and the impact on society that the distinguished physicist, Fritz Zwicky (1898- 1974), has made. So I am not going to try to serve that injustice, rather I will construct a collage, which are cameos of his life and accomplishments. In this way, you, the reader, will hopefully be left with a sense of his greatness and a desire to learn more about him. -
Variable Star Classification and Light Curves Manual
Variable Star Classification and Light Curves An AAVSO course for the Carolyn Hurless Online Institute for Continuing Education in Astronomy (CHOICE) This is copyrighted material meant only for official enrollees in this online course. Do not share this document with others. Please do not quote from it without prior permission from the AAVSO. Table of Contents Course Description and Requirements for Completion Chapter One- 1. Introduction . What are variable stars? . The first known variable stars 2. Variable Star Names . Constellation names . Greek letters (Bayer letters) . GCVS naming scheme . Other naming conventions . Naming variable star types 3. The Main Types of variability Extrinsic . Eclipsing . Rotating . Microlensing Intrinsic . Pulsating . Eruptive . Cataclysmic . X-Ray 4. The Variability Tree Chapter Two- 1. Rotating Variables . The Sun . BY Dra stars . RS CVn stars . Rotating ellipsoidal variables 2. Eclipsing Variables . EA . EB . EW . EP . Roche Lobes 1 Chapter Three- 1. Pulsating Variables . Classical Cepheids . Type II Cepheids . RV Tau stars . Delta Sct stars . RR Lyr stars . Miras . Semi-regular stars 2. Eruptive Variables . Young Stellar Objects . T Tau stars . FUOrs . EXOrs . UXOrs . UV Cet stars . Gamma Cas stars . S Dor stars . R CrB stars Chapter Four- 1. Cataclysmic Variables . Dwarf Novae . Novae . Recurrent Novae . Magnetic CVs . Symbiotic Variables . Supernovae 2. Other Variables . Gamma-Ray Bursters . Active Galactic Nuclei 2 Course Description and Requirements for Completion This course is an overview of the types of variable stars most commonly observed by AAVSO observers. We discuss the physical processes behind what makes each type variable and how this is demonstrated in their light curves. Variable star names and nomenclature are placed in a historical context to aid in understanding today’s classification scheme. -
William A. Fowler Papers
http://oac.cdlib.org/findaid/ark:/13030/kt2d5nb7kj No online items Guide to the Papers of William A. Fowler, 1917-1994 Processed by Nurit Lifshitz, assisted by Charlotte Erwin, Laurence Dupray, Carlo Cossu and Jennifer Stine. Archives California Institute of Technology 1200 East California Blvd. Mail Code 015A-74 Pasadena, CA 91125 Phone: (626) 395-2704 Fax: (626) 793-8756 Email: [email protected] URL: http://archives.caltech.edu © 2003 California Institute of Technology. All rights reserved. Guide to the Papers of William A. Consult repository 1 Fowler, 1917-1994 Guide to the Papers of William A. Fowler, 1917-1994 Collection number: Consult repository Archives California Institute of Technology Pasadena, California Contact Information: Archives California Institute of Technology 1200 East California Blvd. Mail Code 015A-74 Pasadena, CA 91125 Phone: (626) 395-2704 Fax: (626) 793-8756 Email: [email protected] URL: http://archives.caltech.edu Processed by: Nurit Lifshitz, assisted by Charlotte Erwin, Laurence Dupray, Carlo Cossu and Jennifer Stine Date Completed: June 2000 Encoded by: Francisco J. Medina. Derived from XML/EAD encoded file by the Center for History of Physics, American Institute of Physics as part of a collaborative project (1999) supported by a grant from the National Endowment for the Humanities. © 2003 California Institute of Technology. All rights reserved. Descriptive Summary Title: William A. Fowler papers, Date (inclusive): 1917-1994 Collection number: Consult repository Creator: Fowler, William A., 1911-1995 Extent: 94 linear feet Repository: California Institute of Technology. Archives. Pasadena, California 91125 Abstract: These papers document the career of William A. Fowler, who served on the physics faculty at California Institute of Technology from 1939 until 1982. -
Lyman Spitzer 1914–1997
OBITUARIES ried out sonar analysis at Columbia University Lyman Spitzer as a guide to anti-submarine tactics. After the Deaths of Fellows 1914–1997 war, he went back briefly to Yale and in 1947 he was invited to succeed Russell as Professor of Prof. J Wdowczyk yman Spitzer died on 31 March 1997 at Astronomy at Princeton. He accepted, and held Born 28 July 1935 the age of 82. He had a remarkably pro- the post until his formal retirement in 1982. Elected 11 April 1980 Lductive career that spanned quite diverse At Princeton he developed his theories of the Died 6 September 1996 areas of activity and led him to become one of interstellar medium, and the application of his Dr C P Gopalaraman the most influential American scientists of his great knowledge and understanding of physics Born 1 July 1938 time. His personal theoretical contributions to raised the subject to an exciting level. He Elected 13 May 1994 interstellar astronomy and to plasma physics quickly realized that observations of the inter- Died 3 September 1997 quickly established him as a world leader in each stellar gas were most important in the ultra- Mr S Bradford Downloaded from https://academic.oup.com/astrogeo/article/38/6/36/194930 by guest on 24 September 2021 field. He was a pioneer in the opening up of violet where most of the resonance lines of the Born 28 February 1912 common elements lay. This led to a proposal Elected 14 April 1961 for an ultraviolet observatory satellite designed Died ? specifically to study the interstellar medium. -
Ral History Interview with Martin Schwarzschild
An Interview with MARTIN SCHWARZSCHILD OH 124 Conducted by William Aspray on 18 November 1986 Princeton, NJ Charles Babbage Institute Center for the History of Information Processing University of Minnesota, Minneapolis Copyright, Charles Babbage Institute 1 Martin Schwarzschild Interview 18 November 1986 Abstract Schwarzschild describes his early training in automatic computing when he assumed the position of director of the Watson Scientific Computation Laboratory at Columbia University upon the resignation of Wallace Eckert. Schwarzschild describes the computational research he did there on stellar models using advanced IBM tabulating equipment. He next turns to his experience during world war II at Aberdeen Proving Grounds as an enlisted member of the army working on bomb blasts, and mentions work of R. H. Kent, L. Dederick, IBM personnel, John von Neumann, and other scientific consultants on the design of new automatic calculating equipment for the laboratories. Schwarzschild answers questions about the relationship between Kent and von Neumann. His final topic is the work during the 1950s he undertook on stellar interiors using the Institute for Advanced Study computer. He describes his experiences trying to use the computer for large scientific purposes, and recalls the reception of his computational research by the professional astronomy journals. 2 MARTIN SCHWARZSCHILD INTERVIEW DATE: 18 November 1986 INTERVIEWER: William Aspray LOCATION: Princeton, NJ ASPRAY: This is an interview on the 18th of November, 1986 with Martin Schwarzschild in his office at Princeton University. The interviewer is William Aspray of the Charles Babbage Institute. Let's begin by talking about your contacts with von Neumann during the second world war. -
JRASC, October 2002 Issue (PDF)
Publications and Products of October/octobre 2002 Volume/volume 96 Number/numéro 5 [696] The Royal Astronomical Society of Canada Observer’s Calendar — 2003 This calendar was created by members of the RASC. All photographs were taken by amateur astronomers using ordinary camera lenses and small telescopes and represent a wide spectrum of objects. An informative caption accompanies every photograph. The Journal of the Royal Astronomical Society of Canada Le Journal de la Société royale d’astronomie du Canada It is designed with the observer in mind and contains comprehensive astronomical data such as daily Moon rise and set times, significant lunar and planetary conjunctions, eclipses, and meteor showers. The 1998, 1999, and 2000 editions each won the Best Calendar Award from the Ontario Printing and Imaging Association (designed and produced by Rajiv Gupta). Price: $15.95 (members); $17.95 (non-members) (includes postage and handling; add GST for Canadian orders) The Beginner’s Observing Guide This guide is for anyone with little or no experience in observing the night sky. Large, easy to read star maps are provided to acquaint the reader with the constellations and bright stars. Basic information on observing the Moon, planets and eclipses through the year 2005 is provided. There is also a special section to help Scouts, Cubs, Guides, and Brownies achieve their respective astronomy badges. Written by Leo Enright (160 pages of information in a soft-cover book with otabinding that allows the book to lie flat). Price: $15 (includes taxes, postage and handling) Looking Up: A History of the Royal Astronomical Society of Canada Published to commemorate the 125th anniversary of the first meeting of the Toronto Astronomical Club, “Looking Up — A History of the RASC” is an excellent overall history of Canada’s national astronomy organization. -
Full Issue 2016 (Volume 10)
Inklings Forever: Published Colloquium Proceedings 1997-2016 Volume 10 A Collection of Essays Presented at the Tenth Frances White Ewbank Colloquium on Article 54 C.S. Lewis & Friends 6-5-2016 Full Issue 2016 (Volume 10) Follow this and additional works at: https://pillars.taylor.edu/inklings_forever Part of the English Language and Literature Commons, History Commons, Philosophy Commons, and the Religion Commons Recommended Citation (2016) "Full Issue 2016 (Volume 10)," Inklings Forever: Published Colloquium Proceedings 1997-2016: Vol. 10 , Article 54. Available at: https://pillars.taylor.edu/inklings_forever/vol10/iss1/54 This Full Issue is brought to you for free and open access by the Center for the Study of C.S. Lewis & Friends at Pillars at Taylor University. It has been accepted for inclusion in Inklings Forever: Published Colloquium Proceedings 1997-2016 by an authorized editor of Pillars at Taylor University. For more information, please contact [email protected]. Full Issue 2016 (Volume 10) Cover Page Footnote This file is not paginated the same as the print journal. Contact [email protected] if you need additional pagination information. This full issue is available in Inklings Forever: Published Colloquium Proceedings 1997-2016: https://pillars.taylor.edu/inklings_forever/vol10/iss1/54 Inklings Forever, Volume X Proceedings from the Frances White Ewbank Colloquium on C. S. Lewis and Friends Joe Ricke and Rick Hill, Editors Copyright © 2017 Taylor University Winged Lion Press Hamden, CT All rights reserved. Except in the case of quotations embodied in critical articles or reviews, no part of this book may be reproduced or transmitted in any form or by any means, electronic or mechanical, including photocopying, recording, or by any information storage or retrieval system, without written permission of the publisher. -
Alfred Fowler, F.R.S
JOURNAL OF THE TRANSACTIONS OF ·@hr t8ittl1ria Jnstitut~, OR, j gilosopbintl ,Sotietu of ®nat ~ritain. SECRI,'TARY: E. WALTER MAUNDER, F.R.A.S. VOL. XLVII. LONDON: (:\8ullliJSl)rlJ ll!) tl)e inJStitutr, 1, <tmtral 3Suill:riugJS, ErJStminJSter, j,,E.) ALL RIGHTS RESBRVER . 1915. 565TH ORDINARY GENERAL MEETING, HELD IN THE CONFERENCE HALL, CENTRAL HALL, WESTMINSTER, ON MONDAY, MARCH lsT, 1915, AT 4.30 P.M. Sm FRANK W. DYSON, F.R.S., ASTRONOMER ROYAL, TOOK THE OHAIR. The Minutes of the preceding Meeting were read and confirmed. The SECRETARY announced the election of the Rev. Martin Anstey and the Rev. G. Campbell Morgan as Members of the Institute. The Rev. Prebendary H. E. Fox, M.A., opened the Meeting and introduced the Lecturer, Professor Alfred Fowler, F.R.S. THE SPECTRA OF STARS AND NEBUL.JE. By Professor A. FOWLER, F.R.S. [ABSTRACT.] HE purpose of this lecture is to give some indication of the T way in which the wonderful power of the spectroscope has been utilised in investigations of the chemistry of stars and nebula\ and of the bearing of such knowledge upon the great question of celestial evolution. The only intelligible message that a star sends to the earth is borne on its rays of light, and it is only by the analysis of such light that we can learn anything at all as to the chemical composition and physical condition of the star. Such an analysis has been rendered possible by the invention of the spectroscope in its various forms. Each element, and some com pounds, has its own distinctive family of spectrum lines or bands, by which it can be identified wherever it occurs in the luminous condition. -
Cumulative Bio-Bibliography University of California, Santa Cruz June 2020
Cumulative Bio-Bibliography University of California, Santa Cruz June 2020 Puragra Guhathakurta Astronomer/Professor University of California Observatories/University of California, Santa Cruz ACADEMIC HISTORY 1980–1983 B.Sc. in Physics (Honours), Chemistry, and Mathematics, St. Xavier’s College, University of Calcutta 1984–1985 M.Sc. in Physics, University of Calcutta Science College; transferred to Princeton University after first year of two-year program 1985–1987 M.A. in Astrophysical Sciences, Princeton University 1987–1989 Ph.D. in Astrophysical Sciences, Princeton University POSITIONS HELD 1989–1992 Member, Institute for Advanced Study, School of Natural Sciences 1992–1994 Hubble Fellow, Astrophysical Sciences, Princeton University 1994 Assistant Astronomer, Space Telescope Science Institute (UPD) 1994–1998 Assistant Astronomer/Assistant Professor, UCO/Lick Observatory, University of California, Santa Cruz 1998–2002 Associate Astronomer/Associate Professor, UCO/Lick Observatory, University of California, Santa Cruz 2002–2003 Herzberg Fellow, Herzberg Institute of Astrophysics, National Research Council of Canada, Victoria, BC, Canada 2002– Astronomer/Professor, UCO/Lick Observatory, University of California, Santa Cruz 2009– Faculty Director, Science Internship Program, University of California, Santa Cruz 2012–2018 Adjunct Faculty, Science Department, Castilleja School, Palo Alto, CA 2015 Visiting Faculty, Google Headquarters, Mountain View, CA 2015– Co-founder, Global SPHERE (STEM Programs for High-schoolers Engaging in Research -
William Alfred Fowler (1911-95)
NEWS AND VIEWS mice have up to 30% fewer DRG neurons kinson's diseases, raising the possibility adult? The answer is probably that they and 30% of DRG neurons normally ex that failure of autocrine survival signalling act locally to regulate the survival and press TrkB, the subset of neurons that fail could contribute to degenerative neuro plasticity of axon terminals16,17. Consis to survive in the BDNF null mice might logical disease. Lastly, it will be of great tent with this view, anti-NGF antibodies normally depend on an autocrine BDNF interest to find out whether the types of prevent collateral sprouting but do not loop. Importantly, DRG neurons from adult neurons that are normally able to induce death of adult DRG neurons17. the BDNF null mice were used to confirm promote their own survival by an auto The relative importance of autocrine that the effect of the antisense oligo crine mechanism are better able to survive and target-derived survival signalling in nucleotides depended on the expression and regenerate their axons after injury. the nervous system may not become clear of BDNF and that the oligonucleotides The findings of Acheson et al. suggest a for some time, but some basic mechanistic were not nonspecifically toxic. Taken simple explanation as to why developing questions can be addressed in the near together, these results indicate that a sensory neurons switch from a target future. For instance, does the autocrine subset of adult sensory neurons can sus derived to an autocrine supply of survival Iigandlreceptor interaction require that tain their own survival in vitro, and prob factors. -
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.