Guide to the Subrahmanyan Chandrasekhar Papers 1913-2011

Total Page:16

File Type:pdf, Size:1020Kb

Guide to the Subrahmanyan Chandrasekhar Papers 1913-2011 University of Chicago Library Guide to the Subrahmanyan Chandrasekhar Papers 1913-2011 © 2006 University of Chicago Library Table of Contents Descriptive Summary 3 Information on Use 3 Access 3 Citation 3 Biographical Note 4 Scope Note 5 Related Resources 9 Subject Headings 9 INVENTORY 10 Series I: Personal Correspondence and Papers 10 Subseries 1: Biographical materials and personal papers 10 Subseries 2: Personal correspondence 12 Series II: Scientific Correspondence 20 Series III: Scientific Writings 45 Series IV: Lecture Notes 122 Subseries 1: Cambridge University notes 122 Subseries 2: University of Chicago Notes 124 Subseries 3: Special lectures 130 Series V: Astrophysical Journal Records 134 Series VI: Articles by Colleagues 136 Subseries 1: Offprints 136 Subseries 2: Typescripts 136 Series VII: Addenda 137 Subseries 1: Personal and Biographical 140 Sub-subseries 1: General personal and biographical papers 140 Sub-subseries 2: Personal correspondence 154 Sub-subseries 3: Publications 158 Sub-subseries 4: Chandra X-Ray Observatory 163 Subseries 2: Correspondence 164 Subseries 3: Writing 193 Subseries 4: Writings about Chandrasekhar 223 Subseries 5: Writings by others 229 Subseries 6: Audiovisual 239 Sub-subseries 1: Photographic material 239 Sub-subseries 2: Audio 267 Sub-subseries 3: Video 275 Subseries 7: Oversize 276 Subseries 8: Artifacts and framed items 292 Subseries 9: Medals 295 Subseries 10: Restricted 297 Sub-subseries 1: Administrative records and referee’s reports 297 Sub-subseries 2: Financial records 297 Sub-subseries 3: Letters of recommendation for colleagues and faculty appointment301 material Sub-subseries 4: Student grades and letters of recommendation 305 Descriptive Summary Identifier ICU.SPCL.CHANDRASEKHAR Title Chandrasekhar, Subrahmanyan. Papers Date 1913-2011 Size 342 boxes Repository Special Collections Research Center University of Chicago Library 1100 East 57th Street Chicago, Illinois 60637 U.S.A. Abstract Subrahmanyan Chandrasekhar (1910-1995), Astrophysicist, Nobel Prize winner. The Subrahmanyan Chandrasekhar Papers contains personal and professional correspondence, notes, manuscripts, offprints, lecture notes, scientific writings, records of the Astrophysical Journal, awards, honorary degrees, biographical material, photographs, and sound and video recordings. The Papers span Chandrasekhar's career and document his student years at Cambridge University, his teaching career at the University of Chicago, scientific research and writing in astrophysics, editing of the Astrophysical Journal, and connections with family members and friends in India. The Papers document the development of the Department of Astronomy and Astrophysics and Yerkes Observatory, and provide much information on colleagues and students from the late 1930s to the early 1990s. Information on Use Access The collection is open for research, with the exception of Series VII, Subseries X, which contains material to which access is restricted. Sub-subseries 1, Administrative records and referee's reports, contains records that are closed for 30 years from their date of creation. Sub-subseries 2, Financial records, are closed for 50 years from the date of the record's creation. Sub-subseries 3, Letters of Recommendation for Colleagues and faculty appointment material, are closed for 50 years from the date of creation. Sub-subseries 4, Student Grades and Letters of Recommendation, are closed for 80 years from the date of creation. The audio and video material in Series VII, Subseries 6 do not contain access copies. Researchers will need to consult with staff before requesting these items. Citation 3 When quoting material from this collection, the preferred citation is: Chandrasekhar, Subrahmanyan. Papers, [Box #, Folder #], Special Collections Research Center, University of Chicago Library Biographical Note Subrahmanyan Chandrasekhar, astrophysicist, was born October 19, 1910, in Lahore, India (now Pakistan). Originally from southern India, his family returned to Madras in 1918, where Chandrasekhar received most of his schooling. He received a B.A. honors degree from Presidency College, Madras University, in 1930, and Ph.D. and Sc.D. degrees from Cambridge University in 1933 and 1942. While at Cambridge he studied with R. H. Fowler, P. A. M. Dirac, and E. A. Milne, and also spent periods of time with Niels Bohr in Copenhagen and Max Born at Göttingen. He was appointed a Fellow of Trinity College in 1933. In 1936 Chandrasekhar traveled to the U.S. to give lectures at Harvard College Observatory and at Yerkes Observatory of the University of Chicago. Offered positions at both places, he decided to accept the offer from Chicago. He returned to India briefly that year, and in September married Lalitha Doraiswamy, a former classmate at Presidency College. Chandrasekhar came to Yerkes Observatory in January 1937 as a Research Associate. He was made an Assistant Professor in 1938, Associate Professor in 1942, Professor in 1944, and Distinguished Service Professor in 1946. In 1952 he was named Morton D. Hull Distinguished Service Professor of Theoretical Astrophysics. His appointment was expanded to include not only the Department of Astronomy and Astrophysics but also the Department of Physics and the Enrico Fermi Institute of Nuclear Studies. Chandrasekhar also accepted the position of managing editor of the Astrophysical Journal in 1952, and served in that capacity until 1971. His duties often required him to commute from Yerkes to the University campus for several days each week, which he did until 1964 when he moved his permanent residence to Chicago. Although offered positions at other universities many times, he remained at the University of Chicago throughout his career, and continued to teach and do research well past normal retirement age. He and Lalitha became United States citizens in 1953. Early in the 1930s Chandrasekhar developed a theory concerning white dwarf stars, combining Fowler's use of the new quantum statistics with special relativity. He derived the so-called "Chandrasekhar limit," which set a maximum mass beyond which a star could not remain at the white dwarf stage, but would continue collapsing indefinitely. The theory drew immediate and intense opposition from Arthur S. Eddington and other astronomers, and was not fully accepted until over 20 years later, when it became one of the key elements in the formation of ideas concerning neutron stars and black holes. Frustrated by the negative response to his work, but certain of its correctness, Chandrasekhar wrote up his research and published it as An Introduction to the Study of Stellar Structures (1939) then moved on to other topics. A pattern emerged in Chandrasekhar's work, of researching a subject, writing a series of articles, compiling a book, then changing fields, roughly every 10 years. This, combined with his position 4 on the editorial staff of the Astrophysical Journal, gave him a breadth of knowledge and interest. The contributions Chandrasekhar made to various fields can be seen from the titles of his books: Principles of Stellar Dynamics (1942); Radioactive Transfer (1950); Hydrodynamic and Hydromagnetic Stability (1961); Ellipsoidal Figures of Equilibrium (1969); The Mathematical Theory of Black Holes (1983); and Eddington: The Most Distinguished Astrophysicist of His Time (1983). Among the many citations Chandrasekhar received are the Bruce Gold Medal of the Astronomical Society of the Pacific, the Gold Medal of the Royal Astronomical Society of London, the Rumford Prize of the American Academy of Arts and Sciences, the Royal Medal of the Royal Society of London, the National Medal of Science of the United States, and the Padma Vibhushan award of India. In 1983 Chandrasekhar was awarded the Nobel Prize in Physics. He died in Chicago on August 21, 1995. Scope Note The papers of Subrahmanyan Chandrasekhar include personal and professional correspondence, notes, manuscripts, and offprints of published and unpublished scientific writings, lecture notes, records of the Astrophysical Journal, recordings of interviews and other biographical materials. The papers span Chandrasekhar's career and document his student years at Cambridge University, his teaching career at the University of Chicago, scientific research and writing in astrophysics, editing of the Astrophysical Journal, and connections with family members and friends in India. Because of his long tenure at the University of Chicago, Chandrasekhar's papers constitute an important source for documenting the development of the Department of Astronomy and Astrophysics and Yerkes Observatory, and provide much information on colleagues and students from the late 1930s to the early 1980s. Chandrasekhar carefully maintained files of correspondence, manuscripts, and notes throughout his life, as can be seen in the extensive and continuous runs of materials preserved in the collection. The papers have been arranged in seven series. Series VII is an Addenda to the main body of papers and should be consulted for material that complements items in the earlier series. Series I: Personal Correspondence and Papers begins with general biographical materials and miscellaneous personal papers. The first item is "A Scientific Autobiography, 1943-1983," in which Chandrasekhar gives a detailed account of his research and how various projects developed. Following this are lists of degrees, memberships, and awards publications travels and research and lectures completed by year. Among the other papers in this
Recommended publications
  • PDF of Final Newspaper
    Faculty members What began with Commuters: INSIDE honored for graduate Superphone in 1981, Put down your car teaching says ‘Goodbye’ today keys and step off THIS ISSUE that bus Page 3 Page 8 Page 7 THURSDAY, JUNE 11, 2009 VOL. 28 / NO. 18 Farewell ... to print Chronicle’s 28-year run ends today, as news delivery evolves As the University prepares slated for fall 2009, and it will a new generation of electronic provide a platform for a family publications for faculty, staff, of new reports tailored to the students and friends, the interests of different segments University of Chicago Chronicle is of the University community, publishing its final issue. outside media and interested The University News Office observers around the world. In launched the Chronicle 28 years a world increasingly accustomed ago as a way to speak directly to to instant information, all these the University community, at improvements offer timely news a time when newspapers were and updates. a firmly established habit and “We are providing more print provided one of the most information about the University, Artist renderings courtesy of Hoerr Schaudt economical ways to reach a large to more people, in more ways An artist’s renderings provide a view looking west of the current and proposed changes to the streets and number of people. than ever before,” said Julie walkways on the Main Quadrangles. But reading habits have Peterson, Vice President for changed dramatically in recent Communications. “With that years. A survey of Chronicle comes an unprecedented effort to readers this spring showed that 96 reach out to our most important Summer project aimed at making Main percent get some or most of their constituents, the University news from the Internet.
    [Show full text]
  • Al-Nahl Volume 13 Number 3
    Q3/2003 Vol. 13 No. 3 Al-Nahl A Quarterly Publication of Majlis Ansarullah, U.S.A. Baitul-Futuh: Islamic jewel in the heart of England. Exterior and Interior views. Special Issue of the Al-Nahl on the Life of Hadrat Dr. Mufti Muhammad Sadiq, radiyallahu ‘anhu. 60 pages, $2. Special Issue on Dr. Abdus Salam. 220 pages, 42 color and B&W pictures, $3. Ansar Ansar (Ansarullah News) is published monthly by Majlis Ansarullah U.S.A. and is sent free of charge to all Ansar in the U.S. Ordering Information: Send a check or money order in the indicated amount along with your order to Chaudhary Mushtaq Ahmad, 15000 Good Hope Rd, Silver Spring, MD 20905. Price includes shipping and handling within the continental U.S. Conditions of Bai‘at, Pocket-Size Edition Majlis Ansarullah, U.S.A. has published the ten conditions of initiation into the Ahmadiyya Muslim Community in pocket size brochure. Contact your local officials for a free copy or write to Ansar Publications, 15000 Good Hope Rd, Silver Spring MD 20905. Razzaq and Farida A story for children written by Dr. Yusef A. Lateef. Children and new Muslims, all can read and enjoy this story. It makes a great gift for the children of Ahmadi, Non-Ahmadi and Non- Muslim relatives, friends and acquaintances. The book contains colorful drawings. Please send $1.50 per copy to Chaudhary Mushtaq Ahmad, 15000 Good Hope Rd, Silver Spring, MD 20905 with your mailing address and phone number. Majlis Ansarullah U.S.A. will pay the postage and handling within the continental U.S.
    [Show full text]
  • Hendrik Antoon Lorentz's Struggle with Quantum Theory A. J
    Hendrik Antoon Lorentz’s struggle with quantum theory A. J. Kox Archive for History of Exact Sciences ISSN 0003-9519 Volume 67 Number 2 Arch. Hist. Exact Sci. (2013) 67:149-170 DOI 10.1007/s00407-012-0107-8 1 23 Your article is published under the Creative Commons Attribution license which allows users to read, copy, distribute and make derivative works, as long as the author of the original work is cited. You may self- archive this article on your own website, an institutional repository or funder’s repository and make it publicly available immediately. 1 23 Arch. Hist. Exact Sci. (2013) 67:149–170 DOI 10.1007/s00407-012-0107-8 Hendrik Antoon Lorentz’s struggle with quantum theory A. J. Kox Received: 15 June 2012 / Published online: 24 July 2012 © The Author(s) 2012. This article is published with open access at Springerlink.com Abstract A historical overview is given of the contributions of Hendrik Antoon Lorentz in quantum theory. Although especially his early work is valuable, the main importance of Lorentz’s work lies in the conceptual clarifications he provided and in his critique of the foundations of quantum theory. 1 Introduction The Dutch physicist Hendrik Antoon Lorentz (1853–1928) is generally viewed as an icon of classical, nineteenth-century physics—indeed, as one of the last masters of that era. Thus, it may come as a bit of a surprise that he also made important contribu- tions to quantum theory, the quintessential non-classical twentieth-century develop- ment in physics. The importance of Lorentz’s work lies not so much in his concrete contributions to the actual physics—although some of his early work was ground- breaking—but rather in the conceptual clarifications he provided and his critique of the foundations and interpretations of the new ideas.
    [Show full text]
  • 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.
    [Show full text]
  • Einstein's Mistakes
    Einstein’s Mistakes Einstein was the greatest genius of the Twentieth Century, but his discoveries were blighted with mistakes. The Human Failing of Genius. 1 PART 1 An evaluation of the man Here, Einstein grows up, his thinking evolves, and many quotations from him are listed. Albert Einstein (1879-1955) Einstein at 14 Einstein at 26 Einstein at 42 3 Albert Einstein (1879-1955) Einstein at age 61 (1940) 4 Albert Einstein (1879-1955) Born in Ulm, Swabian region of Southern Germany. From a Jewish merchant family. Had a sister Maja. Family rejected Jewish customs. Did not inherit any mathematical talent. Inherited stubbornness, Inherited a roguish sense of humor, An inclination to mysticism, And a habit of grüblen or protracted, agonizing “brooding” over whatever was on its mind. Leading to the thought experiment. 5 Portrait in 1947 – age 68, and his habit of agonizing brooding over whatever was on its mind. He was in Princeton, NJ, USA. 6 Einstein the mystic •“Everyone who is seriously involved in pursuit of science becomes convinced that a spirit is manifest in the laws of the universe, one that is vastly superior to that of man..” •“When I assess a theory, I ask myself, if I was God, would I have arranged the universe that way?” •His roguish sense of humor was always there. •When asked what will be his reactions to observational evidence against the bending of light predicted by his general theory of relativity, he said: •”Then I would feel sorry for the Good Lord. The theory is correct anyway.” 7 Einstein: Mathematics •More quotations from Einstein: •“How it is possible that mathematics, a product of human thought that is independent of experience, fits so excellently the objects of physical reality?” •Questions asked by many people and Einstein: •“Is God a mathematician?” •His conclusion: •“ The Lord is cunning, but not malicious.” 8 Einstein the Stubborn Mystic “What interests me is whether God had any choice in the creation of the world” Some broadcasters expunged the comment from the soundtrack because they thought it was blasphemous.
    [Show full text]
  • Department of Physics and Astronomy 1
    Department of Physics and Astronomy 1 PHSX 216 and PHSX 236, provide a calculus-based foundation in Department of Physics physics for students in physical science, engineering, and mathematics. PHSX 313 and the laboratory course, PHSX 316, provide an introduction and Astronomy to modern physics for majors in physics and some engineering and physical science programs. Why study physics and astronomy? Students in biological sciences, health sciences, physical sciences, mathematics, engineering, and prospective elementary and secondary Our goal is to understand the physical universe. The questions teachers should see appropriate sections of this catalog and major addressed by our department’s research and education missions range advisors for guidance about required physics course work. Chemistry from the applied, such as an improved understanding of the materials that majors should note that PHSX 211 and PHSX 212 are prerequisites to can be used for solar cell energy production, to foundational questions advanced work in chemistry. about the nature of mass and space and how the Universe was formed and subsequently evolved, and how astrophysical phenomena affected For programs in engineering physics (http://catalog.ku.edu/engineering/ the Earth and its evolution. We study the properties of systems ranging engineering-physics/), see the School of Engineering section of the online in size from smaller than an atom to larger than a galaxy on timescales catalog. ranging from billionths of a second to the age of the universe. Our courses and laboratory/research experiences help students hone their Graduate Programs problem solving and analytical skills and thereby become broadly trained critical thinkers. While about half of our majors move on to graduate The department offers two primary graduate programs: (i) an M.S.
    [Show full text]
  • Guide to the Michael Danos Papers 1950-2003
    University of Chicago Library Guide to the Michael Danos Papers 1950-2003 © 2007 University of Chicago Library Table of Contents Descriptive Summary 3 Information on Use 3 Access 3 Citation 3 Biographical Note 3 Scope Note 4 Related Resources 4 Subject Headings 4 INVENTORY 5 Series I: Personal Materials 5 Series II: Research and Writing 7 Series III: Lectures & Conferences 12 Series IV: Reprints 14 Series V: Restricted Materials 15 Series VI: Oversize Documents 19 Descriptive Summary Identifier ICU.SPCL.MDANOS Title Danos, Michael. Papers Date 1950-2003 Size 15.75 linear feet (29 boxes) Repository Special Collections Research Center University of Chicago Library 1100 East 57th Street Chicago, Illinois 60637 U.S.A. Abstract Michael Danos was a theoretical physicist who worked in photonuclear physics, relativistic heavy ions and x-ray imaging devices, and spent several years as a Visiting Scholar at the Enrico Fermi Institute. The Michael Danos Papers consist of 15.75 linear feet of correspondence, calendars, writings, notebooks, clippings, transparencies, conference materials, photographs, blueprints and diagrams, and computer disks. Information on Use Access Series V (Boxes 20-28) contains restricted material. Much of this material contains legal correspondence, and is therefore restricted indefinitely. Box 28 contains computer disks in obsolescent formats; access requires staff review and possible reformatting. The remainder of the collection is unrestricted and open for research. Citation When quoting material from this collection, the preferred citation is: Danos, Michael. Papers [Box #, Folder #], Special Collections Research Center, University of Chicago Library Biographical Note Michael Danos was born in Latvia in 1922, the son of a Hungarian opera singer stranded in that country by the outbreak of World War I.
    [Show full text]
  • Urdu Syllabus
    TUMKUR UINIVERSITY DEPARTMENT OF URDU'. SYLLABUS AND TEXT BOOKS UNDER CBCS SCHEME LANGUAGE URDU lst Semester B.A./llsc/B.com/BBM/BCA lffect From 20!6-tz lst Semester B.A. Svllabus: Texts: I' 1. Collection of Prose and Poetry Urdu Language Text Book for First Semister B.A.: Edited by: URDU BOS (UG) (Printed and Published by prasaranga, Bangarore university, Bangalore) 2. Non-detail : Selected 4 Chapters From Text Book Reference Books: 1. Yadgaray Hali Saleha Aabid Hussain 2. lqbal Ka Narang QopiChandt 'i Page 1 z' i!. .F}*$T g_€.9f.*g.,,,E B'A BE$BEE CBU R$E Eenlcprqrerlh'ed:.Ufifi9 TFXT B €KeCn e,A I SEMESTER, : ,1 1;5:. -ll-=-- -i- - 1. padiye Gar Bcemar. 'M,tr*hf ag:A.hmgd-$tib.uf i 1.,gglrEdnre:a E*yl{arsfrt$ay Khwaja Hasan Nizarni 3" M_ugalrnanen Ki GurashthaTaleem Shibll Nomani +. lfilopatra N+y,Ek Moti €hola Sclence Ki Duniya : 5. g,€land:|4i$ ..- Manarir,Aashiq flarganvi PelfTR.Y i X., Hazrathfsmail Ki Viladat .FJafeez,J*lan*ari Naath 2. Hsli Mir.*e6halib 3. lqbal 4. T*j &Iahat 5*-e-ubipe.t{i Saher Ludhianawi ,,, lqbal, Amjad, Akbar {Z Eaehf 6g'**e€{F} i ': 1.. 6azaf W*& 2;1 ' 66;*; JaB:Flis,qf'*kfiit" 4., : €*itrl $hmed Fara:, 4. €azgl Firaq ,5; *- ,Elajrooh 6, Gqzal Shahqr..Y.aar' V. Gazal tiiarnsp{.4i1sruu ' 8. Gaal Narir Kqgrnt NG$I.SE.f*IL.: 1- : .*akF*!h*s ,&ri*an Ch*lrdar; 3. $alartrf,;oat &jendar.Sixgir.Ee t 3-, llfar*€,Ffate Tariq.€-hil*ari 4',,&alandar t'- €hig*lrl*tn:Ftyder' Ah*|.,9 .
    [Show full text]
  • Inspec Archive - List of Journals Covered Between 1898 and 1968
    February 2006 www.iee.org/inspec Inspec Archive - List of Journals Covered between 1898 and 1968 Abhandlungen der Berlin Akademie Acta Universitatis Lundensis. Sectio II. Medica, Abhandlungen der Braunschweigischen Mathematica, Scientiae Rerum Naturalium Wissenschaftlichen Gesellschaft Acta Universitatis Tamperensis Abhandlungen der Deutschen Akademie der Acustica Wissenschaften zu Berlin, Klasse fur Advanced Energy Conversion Mathematik, Physik und Technik Advances in Atomic and Molecular Physics Abhandlungen der Konigliches Preussisches Advances in Electronics Meteorologies Institut Advances in Physics Abhandlungen der Preussischen Akademieder Advances in Theoretical Physics Wissenschaften Advances of Science Accademia delle Scienze, Medico e Naturali, AEG Mitteilungen Ferrara AEG Progress ACEC Journal AEG Zeitung ACEC Review AEI Engineering Acero y Energia AEI Engineering Review Acta Academiae Aboensis, Mathematical AEI Journal of Telecommunications Physics AEI Research Laboratory Reports Acta and Commentationes Universitatis Aerial Age Tartuensis (Dorpatensis) Aerial Age Weekly Acta Automatica Sinica Aeronautical Engineering Review Acta Bolyaiana Aeronautical Journal Acta Chemica Scandinavica Aeronautical Research Council Current Papers Acta Crystallographica Aeronautical Research Council Reports and Acta Electronica Memoranda Acta Electronica Sinica Aeronautics Acta Geophysica Sinica Aeroplane Acta Mathematica Aerospace Engineering Acta Mathematica Sinica Agricultural and Horticultural Engineering Acta Mechanica Abstracts Acta Medica
    [Show full text]
  • 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.
    [Show full text]
  • An Interpretation of Milne Cosmology
    An Interpretation of Milne Cosmology Alasdair Macleod University of the Highlands and Islands Lews Castle College Stornoway Isle of Lewis HS2 0XR UK [email protected] Abstract The cosmological concordance model is consistent with all available observational data, including the apparent distance and redshift relationship for distant supernovae, but it is curious how the Milne cosmological model is able to make predictions that are similar to this preferred General Relativistic model. Milne’s cosmological model is based solely on Special Relativity and presumes a completely incompatible redshift mechanism; how then can the predictions be even remotely close to observational data? The puzzle is usually resolved by subsuming the Milne Cosmological model into General Relativistic cosmology as the special case of an empty Universe. This explanation may have to be reassessed with the finding that spacetime is approximately flat because of inflation, whereupon the projection of cosmological events onto the observer’s Minkowski spacetime must always be kinematically consistent with Special Relativity, although the specific dynamics of the underlying General Relativistic model can give rise to virtual forces in order to maintain consistency between the observation and model frames. I. INTRODUCTION argument is that a clear distinction must be made between models, which purport to explain structure and causes (the Edwin Hubble’s discovery in the 1920’s that light from extra- ‘Why?’), and observational frames which simply impart galactic nebulae is redshifted in linear proportion to apparent consistency and causality on observation (the ‘How?’). distance was quickly associated with General Relativity (GR), and explained by the model of a closed finite Universe curved However, it can also be argued this approach does not actually under its own gravity and expanding at a rate constrained by the explain the similarity in the predictive power of Milne enclosed mass.
    [Show full text]
  • Resolving Hubble Tension with the Milne Model 3
    Resolving Hubble tension with the Milne model* Ram Gopal Vishwakarma Unidad Acade´mica de Matema´ticas Universidad Auto´noma de Zacatecas, Zacatecas C. P. 98068, ZAC, Mexico [email protected] Abstract The recent measurements of the Hubble constant based on the standard ΛCDM cos- mology reveal an underlying disagreement between the early-Universe estimates and the late-time measurements. Moreover, as these measurements improve, the discrepancy not only persists but becomes even more significant and harder to ignore. The present situ- ation places the standard cosmology in jeopardy and provides a tantalizing hint that the problem results from some new physics beyond the ΛCDM model. It is shown that a non-conventional theory - the Milne model - which introduces a different evolution dynamics for the Universe, alleviates the Hubble tension significantly. Moreover, the model also averts some long-standing problems of the standard cosmology, for instance, the problems related with the cosmological constant, the horizon, the flat- ness, the Big Bang singularity, the age of the Universe and the non-conservation of energy. Keywords: Milne model; ΛCDM model; Hubble tension; SNe Ia observations; CMB observations. arXiv:2011.12146v1 [physics.gen-ph] 20 Nov 2020 1 Introduction The Hubble constant H0 is one of the most important parameters in cosmology which mea- sures the present rate of expansion of the Universe, and thereby estimates its size and age. This is done by assuming a cosmological model. However, the two values of H0 predicted by the standard ΛCDM model, one inferred from the measurements of the early Universe and the other from the late-time local measurements, seem to be in sever tension.
    [Show full text]