Interview with Donald E. Osterbrock
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Chandra and His Students at Yerkes Observatory Donald Ε. Osterbrock
J. Astrophys. Astr. (1996) 17, 233–268 Chandra and his students at Yerkes Observatory Donald Ε. Osterbrock University of Chicago/Lick Observatory, University of California, Santa Cruz, California 95064. USA Abstract. S. Chandrasekhar’s interactions with graduate students in his more than a quarter century at Yerkes Observatory are described. His graduate teaching, Ph.D. thesis students, colloquia and colloquium series, and seminar series were all important aspects of this side of his scientific research career. His managing editorship of The Astro- physical Journal, his one experience in observational astrophysics, a second paper he wrote describing some of the early observational work at Yerkes Observatory, and a third on “the case for astronomy” are all discussed. A famous myth about one of his courses is corrected, and the circumstances under which the “S. Candlestickmaker” parody was written are recounted. Chandra’s computers, recruited in the Williams Bay community, are mentioned. A complete or nearly complete table of all the thesis students who received their Ph.D. degrees under his supervision, at Yerkes and on the campus in Chicago up through his last one in Astronomy and Astrophysics in 1973, is presented, with references to their published thesis papers. 1 Introduction Subrahmanyan Chandrasekhar spent more than a quarter of a century at Yerkes Observatory, a large part of his scientific career. While he was in residence there he wrote four books and more than two hundred papers, moved up the academic hierarchy from research associate to distinguished service professor, and became an American citizen. Other papers in this memorial issue of the Journal of Astro- physics and Astronomy summarize and evaluate Chandra’s research in the many different fields of astrophysics in which he successively worked, each written by a distinguished expert in that field. -
Executive Director Yerkes Future Foundation Williams Bay, Wisconsin ABOUT YERKES FUTURE FOUNDATION
POSITION PROFILE Executive Director Yerkes Future Foundation Williams Bay, Wisconsin ABOUT YERKES FUTURE FOUNDATION The mission of the Yerkes Future Foundation (“YFF”) is to preserve and protect Yerkes Observatory, celebrate its history and continue to foster its goals of research, education and astronomical observation by providing the opportunity to engage to all. YFF is positioning itself as a visionary and forward-thinking organization in the world of astronomy and science. In this next chapter, the goal of YFF is to create breakthrough programs and experiences that advance its mission and vision in powerful new ways resulting in new access to astronomy and science education. Yerkes Observatory also seeks to establish itself as a year-round, world-renowned destination by offering unique ways to engage with the historically significant buildings and grounds, history and STEM learning. In this exciting new chapter for the Observatory, YFF seeks to: 1. Be a place of scientific research that re-captures the underlying academic foundations upon which the Observatory was originally conceived. 2. Be a unique and innovative destination of choice to many thousands of people, beginning with the Wisconsin-Illinois region – and extending far beyond, both nationally and internationally. 3. Influence the life outcomes of its visitors, especially young people. 4. Have a national and international profile – based on a deliberate and intelligent blend of academic and research programs, plus being a thoroughly enjoyable place to visit, either as a casual tourist or as a well-informed seeker of knowledge and adventure. 5. Have educational programs that change people’s viewpoints and thinking and are so profound they are personally motivated to do more – and to share their knowledge with the wider world. -
*Revelle, Roger Baltimore 18, Maryland
NATIONAL ACADEMY OF SCIENCES July 1, 1962 OFFICERS Term expires President-Frederick Seitz June 30, 1966 Vice President-J. A. Stratton June 30, 1965 Home Secretary-Hugh L. Dryden June 30, 1963 Foreign Secretary-Harrison Brown June 30, 1966 Treasurer-L. V. Berkner June 30, 1964 Executive Officer Business Manager S. D. Cornell G. D. Meid COUNCIL *Berkner L. V. (1964) *Revelle, Roger (1965) *Brown, Harrison (1966) *Seitz, Frederick (1966) *Dryden, Hugh L. (1963) *Stratton, J. A. (1965) Hutchinson, G. Evelyn (1963) Williams, Robley C. (1963) *Kistiakowsky, G. B. (1964) Wood, W. Barry, Jr. (1965) Raper, Kenneth B. (1964) MEMBERS The number in parentheses, following year of election, indicates the Section to which the member belongs, as follows: (1) Mathematics (8) Zoology and Anatomy (2) Astronomy (9) Physiology (3) Physics (10) Pathology and Microbiology (4) Engineering (11) Anthropology (5) Chemistry (12) Psychology (6) Geology (13) Geophysics (7) Botany (14) Biochemistry Abbot, Charles Greeley, 1915 (2), Smithsonian Institution, Washington 25, D. C. Abelson, Philip Hauge, 1959 (6), Geophysical Laboratory, Carnegie Institution of Washington, 2801 Upton Street, N. W., Washington 8, D. C. Adams, Leason Heberling, 1943 (13), Institute of Geophysics, University of Cali- fornia, Los Angeles 24, California Adams, Roger, 1929 (5), Department of Chemistry and Chemical Engineering, University of Illinois, Urbana, Illinois Ahlfors, Lars Valerian, 1953 (1), Department of Mathematics, Harvard University, 2 Divinity Avenue, Cambridge 38, Massachusetts Albert, Abraham Adrian, 1943 (1), 111 Eckhart Hall, University of Chicago, 1118 East 58th Street, Chicago 37, Illinois Albright, William Foxwell, 1955 (11), Oriental Seminary, Johns Hopkins University, Baltimore 18, Maryland * Members of the Executive Committee of the Council of the Academy. -
Uchicago April Overnight
THURSDAY AND FRIDAY OVERVIEW (CONT’D) THURSDAY, APRIL 6 (CONT’D) FRIDAY OVERVIEW UCIE: ENTREPRENEURSHIP LUGGAGE DROP-OFF 8:30 a.m. LIBRARY, LUNCH Jerry Huang, Senior Program Director of Drop off your luggage with our staff, and we’ll UChicago Careers in Entrepreneurship, will ROCKEFELLER – IDA NOYES Boxed lunches will be provided to all guests THIRD FLOOR 12:30 p.m. MEMORIAL 2:00 p.m. take care of it for you during the program. Please HALL 11:30 a.m. between 11:30 a.m. and 2:30 p.m. in the three THEATER, lead a panel of students who have started their CHAPEL retrieve all luggage no later than 2:00 p.m. – WEST LOUNGE, 2:30 p.m. locations available. You may go to any of these OR EAST LOUNGE, own businesses with the help of our Career areas located on the second and third floors of IDA NOYES HALL Advancement office. Ida Noyes Hall. (Thursday only.) SCHEDULE OF EVENTS: FRIDAY, APRIL 7 MODEL CLASS: ASTROPHYSICS MAX P. Richard Kron is a Professor of Astronomy and CINEMA, ECONOMICS INFORMATION SESSION Astrophysics and the College, and is the former IDA NOYES HALL Grace Tsiang, Senior Lecturer and Co-Director of Director of the Yerkes Observatory. STUDENTS MEET OVERNIGHT HOSTS Undergraduate Studies in Economics, will give ROCKEFELLER 9:30 a.m. MEMORIAL All students staying overnight must attend MAX P. CINEMA, 4:15 p.m. an overview of academic resources and research CHAPEL this session. Please note: This session is for IDA NOYES HALL opportunities in our incomparable economics students only. -
Back Bay Amateur Astronomers P.O
BACKBACK BAYBAY observerobserver The Official Newsletter of the Back Bay Amateur Astronomers P.O. Box 9877, Virginia Beach, VA 23450-9877 Looking Up! Greetings once again skywatchers! The annual EPHEMERALS Astronomical League Conference (ALCon) is this july 2012 month in Chicago, and I will be attending. We, as a club, are a part of the Astronomical League and are entitled to all the benefits included. For those of you who don’t 07/13 know, the Astronomical League is made up of many of Skywatch the astronomy clubs across the nation. They sponsor Northwest River Park many observing programs, such as the Messier Program, the Binocular Program, the Planetary Nebula 07/14, 11:00 am Program (which BBAA helped begin) and awards such BBAA Family Picnic as the National Young Astronomer Award, the Horkheimer/Smith Award, and many, many more. Northwest River Park They also publish a quarterly newsletter called The Large Picnic Shelter Reflector that every member receives. 07/20, 7:00 pm Back to ALCon, it’s like any other conference except there’s a bunch of astronomer nerds hanging out and Night Hike talking about astronomer stuff. There are speakers, Northwest River Park events and day trips. For example, this year there are trips to Yerkes Observatory, Fermilab, and the Adler 07/21 Planetarium. There will also be nightly star parties, a Nightwatch “Star-B-Que” and an awards banquet. It’s going to be Chippokes State Park bunches of fun and I’m sure I will have many stories to Surry, VA tell when I come back. -
How Supernovae Became the Basis of Observational Cosmology
Journal of Astronomical History and Heritage, 19(2), 203–215 (2016). HOW SUPERNOVAE BECAME THE BASIS OF OBSERVATIONAL COSMOLOGY Maria Victorovna Pruzhinskaya Laboratoire de Physique Corpusculaire, Université Clermont Auvergne, Université Blaise Pascal, CNRS/IN2P3, Clermont-Ferrand, France; and Sternberg Astronomical Institute of Lomonosov Moscow State University, 119991, Moscow, Universitetsky prospect 13, Russia. Email: [email protected] and Sergey Mikhailovich Lisakov Laboratoire Lagrange, UMR7293, Université Nice Sophia-Antipolis, Observatoire de la Côte d’Azur, Boulevard de l'Observatoire, CS 34229, Nice, France. Email: [email protected] Abstract: This paper is dedicated to the discovery of one of the most important relationships in supernova cosmology—the relation between the peak luminosity of Type Ia supernovae and their luminosity decline rate after maximum light. The history of this relationship is quite long and interesting. The relationship was independently discovered by the American statistician and astronomer Bert Woodard Rust and the Soviet astronomer Yury Pavlovich Pskovskii in the 1970s. Using a limited sample of Type I supernovae they were able to show that the brighter the supernova is, the slower its luminosity declines after maximum. Only with the appearance of CCD cameras could Mark Phillips re-inspect this relationship on a new level of accuracy using a better sample of supernovae. His investigations confirmed the idea proposed earlier by Rust and Pskovskii. Keywords: supernovae, Pskovskii, Rust 1 INTRODUCTION However, from the moment that Albert Einstein (1879–1955; Whittaker, 1955) introduced into the In 1998–1999 astronomers discovered the accel- equations of the General Theory of Relativity a erating expansion of the Universe through the cosmological constant until the discovery of the observations of very far standard candles (for accelerating expansion of the Universe, nearly a review see Lipunov and Chernin, 2012). -
Reflections December 2020
Surviving the Bobcat Fire By Robert Anderson As recently as December 9, our solar astronomer, Steve Padilla, was taking his evening walk and noticed the smoke of a hotspot flaring up in the canyon just below the Observatory. It was a remnant of the Bobcat Fire, which started nearby on September 6. The local Angeles National Forest firefighters were notified of the flareup, either to monitor it or extinguish it if needed. They have returned many times during the last three months. And we are always glad to see them, especially those individuals who put water to flame here and battled to save the most productive and famous observatory in history. On the sunny Labor Day weekend, when the Bobcat Fire started near Cogswell Reservoir in a canyon east of the Mount Wilson, the Observatory’s maintenance staff went on cautious alert. As the fire spread out of control, it stayed to the east burning north and south of the reservoir for days, threatening communities in the foothills of the San Gabriels. Nevertheless, all non-essential staff and residents were evacuated off the mountain just in case. Under a surreal, smoke-filled September sky, crews David Cendejas, the superintendent of the Observatory, prepare to defend the Observatory. Photo: D. Cendejas and a skeleton crew of CHARA staff, stayed to monitor the situation and to secure the grounds. Routine year- round maintenance of Mount Wilson always includes In this issue . clearing a wide perimeter of combustibles from the buildings, but when a large fire is burning nearby, clearing Surviving the Fire ……………1 Betelgeuse & Baade …………….5 anything that has been missed becomes an urgent priority, News + Notes .….………………2 Thanks to our Supporters! ..….7 along with double-checking all the fire equipment. -
Physicists Look to a New Telescope to Understand Neutron Stars and Matter at the Extremes INNER WORKINGS
Correction INNER WORKINGS Correction for “Inner Workings: Physicists look to a new tele- scope to understand neutron stars and matter at the extremes,” by Stephen Ornes, which was first published November 4, 2020; 10.1073/pnas.2021447117 (Proc.Natl.Acad.Sci.U.S.A.117, 29249–29252). The editors note that ref. 5 appeared incorrectly. It should instead appear as below. The online version has been corrected. 5. E. Annala, T. Gorda, A. Kurkela, J. Nättilä, A. Vuorinen, Evidence for quark-matter cores in massive neutron stars. Nat. Phys. 16, 907–910 (2020). Published under the PNAS license. First published December 21, 2020. www.pnas.org/cgi/doi/10.1073/pnas.2024053117 CORRECTION www.pnas.org PNAS | December 29, 2020 | vol. 117 | no. 52 | 33719 Downloaded by guest on October 2, 2021 INNER WORKINGS Physicists look to a new telescope to understand neutron stars and matter at the extremes INNER WORKINGS Stephen Ornes, Science Writer Astronomers ostensibly know plenty about neutron matter at such high densities has long been a puzzle,” stars: the hot, collapsed remnants of massive stars says Arzoumanian. Now a small, boxy X-ray telescope that have exploded as supernovae. These objects mounted on the International Space Station is spilling can spin up to hundreds of times a second, generate the inner secrets of these stars. Called the Neutron intense magnetic fields, and send out jets of radia- Star Interior Composition Explorer, or NICER, it can tion that sweep the sky like beams from a lighthouse. measure the size and mass of neutron stars, revealing When two neutron stars collide, the ripples in space- their true density. -
Wisconsin Society of Science Teachers Convention 2008
Wisconsin Society of Science Teachers Convention 2008 Report to the HPS Science Support Committee and North Central Chapter • Marcum Martz, Medical College of Wisconsin • Dan Miron, Cardinal Health • Paul Ward, Zablocki VA Medical Center • Paul Schmidt, WI DHFS, Radiation Protection Section WSST held its annual convention March 13-15 in Lake Geneva, Wisconsin. As part of the mission of the HPS Science Support Committee and the NCCHPS to bring health physics to attention of middle schools and high schools, representatives of NCCHPS participated as presenters and exhibitors. The presentations consisted of two one-hour lectures and one three-hour lab workshop. The first lecture was on the topic of the fundamentals of radiation, including basic physics, units and sources of natural and man-made radiation. The nearly completed Power Point presentation by the SSC serves as the model for this lecture, which is well- suited as an introductory primer for middle/high school teachers. The second lecture was Radiation in Research, Medicine and Education. Both of these lectures were well- attended; we ran a little over the schedule due to many excellent questions asked, and much interest was generated. The three-hour lab workshop was less successful, possibly due to circumstances that were beyond our control: 1) the WSST program was accidentally printed with the page describing all the three-hour workshops left blank; no one knew about the workshop unless they pre-registered online. 2) The workshop was scheduled (by WSST) on the same morning of most of the off-site tours to such venues as Fermilab and Yerkes Observatory. -
David Kaplan (University of Wisconsin, Milwaukee) [email protected]
Remote Radio Astronomy: ARCC@UWM David Kaplan (University of Wisconsin, Milwaukee) [email protected] Leonard E. Parker Center for Gravitation, Cosmology & Astrophysics Goals • Integrate students into research at a very early stage, with low initial commitment • Years 1-4, Physics & non-physics • Learn about modern scientific research methods, attract into STEM fields • Offer opportunities for students to gain personal investment in research • Gain assistance in finding new pulsars (still very labor intensive) Arecibo Remote Command Center • Started at University of Texas Brownsville • Part of PALFA pulsar survey • Expanded to UWM in 2008 (X. Siemens): ARCC@UWM • Now at least 3 other universities offer ARCC programs Major Activities 1.Students conduct remote observing at Arecibo and Green Bank radio telescopes as part of pulsar surveys 2.Students examine pulsar candidates to identify “real” signals 3.UWM Astronomy Club: exploration of modern research and cohort formation Candidate Rating Training • Initial lectures in “what is a pulsar” and “radio astronomy basics” • Discussion of what distinguishes real pulsars from other signals • Once trained, students examine pulsar candidates from web interface at home (or elsewhere) • Paid work ($11/hour) Observing Training • Remote observing requires significant training & apprenticeship: • GBT requires on-site, Arecibo does not • Use older students to mentor new students until they are trained and comfortable • Gradual increase in responsibilities ARCC Network • Weekly meetings at each University led by team leader • UWM has 2 teams • Offers leadership opportunities for senior students • Monthly meetings across Universities, including presentations about other science • Space Presentation Outreach Talks (SPOT) delivered to local high schools UWM Astronomy Club • Led by 3 faculty, including non-pulsar researcher • Weekly meetings led by faculty (not students) • Presentations, guest speakers, activities, discussion of news items, etc. -
January 2004 Issue of the OSS Voyages Newsletter
COMMITTEE ON THE STATUS OF MINORITIES IN ASTRONOMY J ANUARY 2004 SPECTRUM A report on underrepresented minorities in astronomy INSIDE THIS ISSUE: So… What About 1 So… What About Diversity? Diversity? by Marcel Agueros Professional Organi- 1 zations of Minorities Led by a team of graduate students, the University of in Physical Sciences Washington Astronomy Department has developed a The Accountability 4 departmental plan for more effectively engaging diver- Side of Diversity sity issues through enhanced coordination of effort and improved leveraging of available resources. What’s in a Name? 6 Marcel Agueros describes how they went about it and Astronomy Faculty 9 what they learned along the way. Diversity Survey: Preliminary Results A Small First Step 10 he meeting was over. For nearly an hour the graduate students and the graduate program ad- Ph.D. Productivity of 12 visor had intensively discussed a number of Historically Black T Colleges pressing departmental issues. We were wrapping up Marcel Agueros is a when a question was casually dropped on the table: 4th-year astronomy SASS: Cultivating the 14 “What about diversity?” graduate student at the Next Generation of University of Washing- Astronomers What seemed like a simple enough question to ask ton. His dissertation NASA Space Science 16 turned out to be a very difficult question to answer. That research is on X-ray Diversity Initiatives meeting took place about a year ago, and we are still selected stars from the working our way to a good answer. However, with the RASS and SDSS Sur- Meet Dara Norman at 17 help of some friends—the Graduate Opportunities and veys under the direc- CTIO Minority Achievement Program and ADVANCE here at tion of Scott Anderson. -
George Willis Ritchey: Astrophotographer by Robert Anderson
S P R I N G Q U A R T E R / M A R C H 2 0 1 9 George Willis Ritchey: Astrophotographer By Robert Anderson A century ago, Mount Wilson Observatory lost a brilliant astronomer — George Willis Ritchey. When George Ellery Hale left Yerkes Observatory in 1904 to create Mount Wilson, Ritchey was one of four staff members he brought with him. Hale knew he would be indispensable to the new endeavor. And Ritchey was. He designed and built almost every early telescope and optical component on the mountain. Yet for all his contributions, a clash of egos with Hale and charges of disloyalty lead to his dismissal on October 31, 1919. The story of this unpleasant affair is well told by astronomer Donald Osterbrock in his 1993 book, Pauper & Prince: Ritchey, Hale, and Big American Telescopes. It is also the best account of the master optician and his genius (from which much of the information in this article is derived). On the centennial of Ritchey’s On ecember th, , eorge itchey took his rst departure, let’s celebrate his amazing work instead. photograph with the new 60-inch Telescope on Mount Wilson. He chose the Orion Nebula. Perhaps the most Ritchey wore many hats. He was an astronomer, a photographed object in the night sky, recording details of telescope designer, and an expert optician. He took the its glowing gases is a true test of an astrophotographer’s technology of mirror grinding to new levels of perfection equipment and skills. Credit: Carnegie Observatories. —such that his 60-inch mirror grinding machine now rests in the Smithsonian.