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Review Section
CSIRO PUBLISHING www.publish.csiro.au/journals/hras Historical Records of Australian Science, 2004, 15, 121–138 Review Section Compiled by Libby Robin Centre for Resource and Environmental Studies (CRES), Australian National University, Canberra, ACT, 0200, Australia. Email: [email protected] Tom Frame and Don Faulkner: Stromlo: loss of what he described as a ‘national an Australian observatory. Allen & Unwin: icon’. Sydney, 2003. xix + 363 pp., illus., ISBN 1 Institutional histories are often suffused 86508 659 2 (PB), $35. with a sense of inevitability. Looking back from the security of a firmly grounded present, the road seems straight and well marked. The journey that is reconstructed is one where the end point is always known, where uncertainties and diversions are forgotten — a journey that lands neatly on the institution’s front doorstep. Institu- tional histories are often burdened, too, by the expectation that they will not merely tell a story, but provide a record of achieve- ment. Written for the institution’s staff, as well as broader public, they can become bogged down in the details of personnel and projects. In this case, the fires of January 2003 add an unexpected final act Few institutional histories could boast such to what is a fairly traditional story of a dramatic conclusion as Stromlo: an Aus- growth and success. The force of nature tralian observatory. The manuscript was intervenes to remind us of the limits of substantially complete when a savage fire- inevitability, to fashion from the end point storm swept through the pine plantations another beginning. flanking Mount Stromlo, destroying all the The book is roughly divided into halves. -
William Liller (1927–2021)
Bulletin of the AAS • Vol. 53, Issue 2 William Liller (1927–2021) Alan Hirshfeld1, Christine Jones2, William Forman2 1UMass Dartmouth, 2Center for Astrophysics | Harvard & Smithsonian Published on: Apr 07, 2021 DOI: 10.3847/25c2cfeb.97f3253d License: Creative Commons Attribution 4.0 International License (CC-BY 4.0) Bulletin of the AAS • Vol. 53, Issue 2 William Liller (1927–2021) William Liller died on Sunday the 28th of February 2021. William (“Bill”) Liller, research mentor and major contributor to the study of planetary nebulae, comets, asteroids, magnetic activity in cool stars, the optical identification of X-ray sources, and astro-archaeology, died peacefully in his sleep on 28 February 2021, after a brief illness. He was 93 years old. Born on 1 April 1927 in Philadelphia to Carroll Kalbaugh “Pete” Liller, an advertising executive, and his wife, Catherine Dellinger Liller, Bill noted in the book “Asteroids to Quasars” that he became “obsessed with astronomy” in Photo courtesy Clive Grainger. August 1932, when his uncle drove up from West Virginia in a Model A Ford to view a solar eclipse from New York, near where Bill’s family was living at the time. At age 13, Bill’s report on the Quadrantid meteor shower was cited in an article in Popular Astronomy from the American Meteor Society. In his letter to the society, Bill had misspelled the name of the society’s director, C. P. Olivier, which Bill believed led to an intentional misspelling of his own name in the published article as “Billy Lillier.” In the February 2018 issue of the alumni magazine of Harvard’s Adams House, Bill recalled the years leading up to his matriculation in 1944: “After attending public schools in my home town of Atlanta, I was shipped off ‘to finish,’ and I spent my last two high school years at Mercersburg Academy in Pennsylvania. -
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. -
Pos(Westerbork)002 Historical Introduction Historical S 4.0 International License (CC BY-NC-ND 4.0)
Historical Introduction PoS(Westerbork)002 Richard Strom ASTRON Oude Hoogeveensedijk 4, 7991 PD Dwingeloo, The Netherlands E-mail: [email protected] 50 Years Westerbork Radio Observatory, A Continuing Journey to Discoveries and Innovations Richard Strom, Arnold van Ardenne, Steve Torchinsky (eds) Published with permission of the Netherlands Institute for Radio Astronomy (ASTRON) under the terms of the Creative CommonsAttribution-NonCommercial-NoDerivatives 4.0 International License (CC BY-NC-ND 4.0). Chapter 1 Historical introduction Richard Strom* rom the English longbows at the battle of Crécy (1346) to Winston Chur- chill’s world war I mobilized cannon (its true identity hidden behind the Fpseudonym “[water] tank”), warfare has always pushed technological innovation to new fronts. The second world war (WWII) was no exception. It gave us technology ranging from the dynamo-powered flashlight (a Philips invention) to jet engines, and space-capable rockets (Germany’s V2), not to mention (in a completely different realm) the mass production of Penicillin. In fact, it could be argued that WWII inventions marked the inception of the modern technological era1. In the field of electronics, the war led to innovations such as radio navigation, aircraft landing systems, and radar. It was these developments which were to * ASTRON, Univer- sity of Amsterdam, have a revolutionary impact on astronomy, initially in Britain, Australia and the The Netherlands United States. But the story begins in the US, with the electronics of the 1920s and ‘30s. Figure 1. Karl G. Jansky (c. 1933) Around 1930, there was increasing interest in the use of radio frequencies for communication. One of the main players, the Bell Telephone Laboratories in New Jersey, asked their research engineer, Karl Jansky (Figure 1), to investigate the inter- ference environment in the “short-wave” band around 20 MHz. -
Illinois—Where Astronomical Photometry Grew Up
Beaman and Svec, JAAVSO Volume 40, 2012 141 Illinois—Where Astronomical Photometry Grew Up Barry B. Beaman 6804 Alvina Road, Rockford, IL 61101; [email protected] Michael T. Svec Furman University, Department of Education, 3300 Poinsett Highway, Greenville SC 29613; Internet: [email protected] Presented at the 100th Annual Meeting of the AAVSO, October 7, 2011; received January 21, 2012; revised February 2, 2012; accepted February 6, 2012 Abstract In 1903 Dr. Joel Stebbins joined the University of Illinois faculty as an astronomy instructor and Director of the University of Illinois Observatory. In 1905 he and F. C. Brown began experimenting with selenium sell photometry and developed the equipment and many of the photometric practices used then. Those practices formed the foundation on which present day photometry processes are based. This paper will trace the history of Stebbins’ career and his development of photoelectric photometry from 1903 to 1922. This story explains how Stebbins’ wife, May, caused a change in astronomical observing that continues today. 1. Introduction The prairies of central Illinois may seem an unlikely place to begin a photometric revolution. Illinois is a flat land state with only about 100 clear nights per year, the average elevation is only 600 feet above sea level, and the highest point is only at 1,500 feet. Yet, Illinois has produced its share of prominent and innovative astronomers. George Ellery Hale built his Kenwood Observatory in the heart of Chicago. Edwin Hubble spent his teen years in the Chicago suburbs and was educated at University of Chicago. Grote Reber built the World’s first parabolic-steerable radio telescope. -
HST Public Lecture Series
WelcomeWelcome toto thethe SpaceSpace TelescopeTelescope ScienceScience InstituteInstitute’’ss PublicPublic LectureLecture SeriesSeries zz YourYour host:host: MaxMax MutchlerMutchler zz LithographsLithographs onon tabletable z PleasePlease taketake oneone perper personperson TONIGHT TransNeptunianTransNeptunian BinariesBinaries andand CollisionCollision Families:Families: ProbesProbes ofof OurOur LocalLocal DustDust DiskDisk SusanSusan BenecchiBenecchi MayMay 5,5, 20092009 88 PMPM STScISTScI AuditoriumAuditorium UpcomingUpcoming TalksTalks zz JuneJune 2,2, 20092009 –– JasonJason TumlinsonTumlinson,, TheThe InvisibleInvisible Galaxy:Galaxy: NewNew ViewsViews ofof thethe MilkyMilky WayWay zz JulyJuly 7,7, 20092009 –– DouglasDouglas Long,Long, TheThe MysteryMystery ofof thethe ‘‘BeBe’’ StarsStars WebWeb SiteSite && WebcastWebcast • Google “hubble lecture” • http://hubblesite.org/go/talks • List of upcoming speakers • Link to current webcast • Links to previous webcasts Scientific Symposium May 4-7 Public Lecture May 8 at 7:00 PM at the Maryland Science Center: Dr. Steven Squyers (Cornell): Roving Mars Hubble Servicing Mission 4 Launch currently set for May 11, 2009 Two Space Shuttles sitting on the launch pad Hubble was deployed and is serviced by the Space Shuttle 1990 1993 1997 1999 2002 2009 5 days of spacewalking! Hubble mission milestones as chronicled by it’s workhorse: Wide Field Planetary Camera 2 (WFPC2, to be replaced with WFC3) “Top 10 reasons why the Hubble telescope isn’t working…” WFPC2 installed during servicing mission 1 -
Investigations of the Interstellar Medium at Washburn Observatory, 1930-58
Journal of Astronomical History andheritage 7(2):85-94 2004 Investigations of the interstellar medium at Washburn Observatory, 1930-58 David S Liebl* University of Wisconsin- College of Engineering, 432 North Lake Street, Rm. 311, Madison, Wisconsin 53706, USA E-mail: [email protected] Christopher Fluke Centre for Astrophysics and Supercomputing, Swinbume University ofTeclmo/ogy, PO Box 218, Victoria 3122, Australia E-mail: [email protected] Abstract Behveen 1930 and 1958, the Washburn Observatory of the University of Wisconsin-Madison was home to pioneering photometric research into the interstellar medium by Joel Stebbins and Albert Whitford. Between 1933 and 1941, Stebbins and Whitford published seminal research on the photometry of stellar reddening, using the Washburn 15-inch refractor and the 60- and 100-inch reflectors at Mount Wilson Observatory. Many factors were responsible for the Washburn Observatory's pre-eminence in this area. l11is paper reviews their research on interstellar dust during the years 1922 58, the observational teclmology and scientific methods that were developed at the Washburn Observatory during that time and the scientific discoveries that originated there. We discuss the factors that enabled WashburnObservatory to become a leader in photometry during the first half of the twentieth century. We also draw on the recollections of past and present Washburn Observatory scientists1 to understand how Washburn's standing led to a subsequent programme of research into the interstellar medium at the University of Wisconsin-Madison. The resulting portrayal of Washburn Observatory provides insights into the evolution of astronomical research in America, from the beginning of the hventieth cenh1ry until today. -
Stars and Their Spectra: an Introduction to the Spectral Sequence Second Edition James B
Cambridge University Press 978-0-521-89954-3 - Stars and Their Spectra: An Introduction to the Spectral Sequence Second Edition James B. Kaler Index More information Star index Stars are arranged by the Latin genitive of their constellation of residence, with other star names interspersed alphabetically. Within a constellation, Bayer Greek letters are given first, followed by Roman letters, Flamsteed numbers, variable stars arranged in traditional order (see Section 1.11), and then other names that take on genitive form. Stellar spectra are indicated by an asterisk. The best-known proper names have priority over their Greek-letter names. Spectra of the Sun and of nebulae are included as well. Abell 21 nucleus, see a Aurigae, see Capella Abell 78 nucleus, 327* ε Aurigae, 178, 186 Achernar, 9, 243, 264, 274 z Aurigae, 177, 186 Acrux, see Alpha Crucis Z Aurigae, 186, 269* Adhara, see Epsilon Canis Majoris AB Aurigae, 255 Albireo, 26 Alcor, 26, 177, 241, 243, 272* Barnard’s Star, 129–130, 131 Aldebaran, 9, 27, 80*, 163, 165 Betelgeuse, 2, 9, 16, 18, 20, 73, 74*, 79, Algol, 20, 26, 176–177, 271*, 333, 366 80*, 88, 104–105, 106*, 110*, 113, Altair, 9, 236, 241, 250 115, 118, 122, 187, 216, 264 a Andromedae, 273, 273* image of, 114 b Andromedae, 164 BDþ284211, 285* g Andromedae, 26 Bl 253* u Andromedae A, 218* a Boo¨tis, see Arcturus u Andromedae B, 109* g Boo¨tis, 243 Z Andromedae, 337 Z Boo¨tis, 185 Antares, 10, 73, 104–105, 113, 115, 118, l Boo¨tis, 254, 280, 314 122, 174* s Boo¨tis, 218* 53 Aquarii A, 195 53 Aquarii B, 195 T Camelopardalis, -
Download the 2016 Spring Deep-Sky Challenge
Deep-sky Challenge 2016 Spring Southern Star Party Explore the Local Group Bonnievale, South Africa Hello! And thanks for taking up the challenge at this SSP! The theme for this Challenge is Galaxies of the Local Group. I’ve written up some notes about galaxies & galaxy clusters (pp 3 & 4 of this document). Johan Brink Peter Harvey Late-October is prime time for galaxy viewing, and you’ll be exploring the James Smith best the sky has to offer. All the objects are visible in binoculars, just make sure you’re properly dark adapted to get the best view. Galaxy viewing starts right after sunset, when the centre of our own Milky Way is visible low in the west. The edge of our spiral disk is draped along the horizon, from Carina in the south to Cygnus in the north. As the night progresses the action turns north- and east-ward as Orion rises, drawing the Milky Way up with it. Before daybreak, the Milky Way spans from Perseus and Auriga in the north to Crux in the South. Meanwhile, the Large and Small Magellanic Clouds are in pole position for observing. The SMC is perfectly placed at the start of the evening (it culminates at 21:00 on November 30), while the LMC rises throughout the course of the night. Many hundreds of deep-sky objects are on display in the two Clouds, so come prepared! Soon after nightfall, the rich galactic fields of Sculptor and Grus are in view. Gems like Caroline’s Galaxy (NGC 253), the Black-Bottomed Galaxy (NGC 247), the Sculptor Pinwheel (NGC 300), and the String of Pearls (NGC 55) are keen to be viewed. -
407 a Abell Galaxy Cluster S 373 (AGC S 373) , 351–353 Achromat
Index A Barnard 72 , 210–211 Abell Galaxy Cluster S 373 (AGC S 373) , Barnard, E.E. , 5, 389 351–353 Barnard’s loop , 5–8 Achromat , 365 Barred-ring spiral galaxy , 235 Adaptive optics (AO) , 377, 378 Barred spiral galaxy , 146, 263, 295, 345, 354 AGC S 373. See Abell Galaxy Cluster Bean Nebulae , 303–305 S 373 (AGC S 373) Bernes 145 , 132, 138, 139 Alnitak , 11 Bernes 157 , 224–226 Alpha Centauri , 129, 151 Beta Centauri , 134, 156 Angular diameter , 364 Beta Chamaeleontis , 269, 275 Antares , 129, 169, 195, 230 Beta Crucis , 137 Anteater Nebula , 184, 222–226 Beta Orionis , 18 Antennae galaxies , 114–115 Bias frames , 393, 398 Antlia , 104, 108, 116 Binning , 391, 392, 398, 404 Apochromat , 365 Black Arrow Cluster , 73, 93, 94 Apus , 240, 248 Blue Straggler Cluster , 169, 170 Aquarius , 339, 342 Bok, B. , 151 Ara , 163, 169, 181, 230 Bok Globules , 98, 216, 269 Arcminutes (arcmins) , 288, 383, 384 Box Nebula , 132, 147, 149 Arcseconds (arcsecs) , 364, 370, 371, 397 Bug Nebula , 184, 190, 192 Arditti, D. , 382 Butterfl y Cluster , 184, 204–205 Arp 245 , 105–106 Bypass (VSNR) , 34, 38, 42–44 AstroArt , 396, 406 Autoguider , 370, 371, 376, 377, 388, 389, 396 Autoguiding , 370, 376–378, 380, 388, 389 C Caldwell Catalogue , 241 Calibration frames , 392–394, 396, B 398–399 B 257 , 198 Camera cool down , 386–387 Barnard 33 , 11–14 Campbell, C.T. , 151 Barnard 47 , 195–197 Canes Venatici , 357 Barnard 51 , 195–197 Canis Major , 4, 17, 21 S. Chadwick and I. Cooper, Imaging the Southern Sky: An Amateur Astronomer’s Guide, 407 Patrick Moore’s Practical -
Atlas Menor Was Objects to Slowly Change Over Time
C h a r t Atlas Charts s O b by j Objects e c t Constellation s Objects by Number 64 Objects by Type 71 Objects by Name 76 Messier Objects 78 Caldwell Objects 81 Orion & Stars by Name 84 Lepus, circa , Brightest Stars 86 1720 , Closest Stars 87 Mythology 88 Bimonthly Sky Charts 92 Meteor Showers 105 Sun, Moon and Planets 106 Observing Considerations 113 Expanded Glossary 115 Th e 88 Constellations, plus 126 Chart Reference BACK PAGE Introduction he night sky was charted by western civilization a few thou - N 1,370 deep sky objects and 360 double stars (two stars—one sands years ago to bring order to the random splatter of stars, often orbits the other) plotted with observing information for T and in the hopes, as a piece of the puzzle, to help “understand” every object. the forces of nature. The stars and their constellations were imbued with N Inclusion of many “famous” celestial objects, even though the beliefs of those times, which have become mythology. they are beyond the reach of a 6 to 8-inch diameter telescope. The oldest known celestial atlas is in the book, Almagest , by N Expanded glossary to define and/or explain terms and Claudius Ptolemy, a Greco-Egyptian with Roman citizenship who lived concepts. in Alexandria from 90 to 160 AD. The Almagest is the earliest surviving astronomical treatise—a 600-page tome. The star charts are in tabular N Black stars on a white background, a preferred format for star form, by constellation, and the locations of the stars are described by charts. -
Assessment of Stellar Stratification in Three Young Star Clusters in The
ACCEPTED FOR PUBLICATION IN THE ASTROPHYSICAL JOURNAL Preprint typeset using LATEX style emulateapj v. 11/10/09 ASSESSMENT OF STELLAR STRATIFICATION IN THREE YOUNG STAR CLUSTERS IN THE LARGE MAGELLANIC CLOUD. DIMITRIOS A. GOULIERMIS Max Planck Institute for Astronomy, Königstuhl 17, 69117 Heidelberg, Germany DOUGAL MACKEY Institute for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill, Edinburgh, EH9 3HJ, UK YU XIN Argelander-Institut für Astronomie, Rheinische Friedrich-Wilhelms-Universität Bonn, Auf dem Hügel 71, 53121 Bonn, Germany AND BOYKE ROCHAU Max Planck Institute for Astronomy, Königstuhl 17, 69117 Heidelberg, Germany Accepted for Publication in the Astrophysical Journal ABSTRACT We present a comprehensive study of stellar stratification in young star clusters in the LargeMagellanicCloud (LMC). We apply our recently developed effective radius method for the assessment of stellar stratification on imaging data obtained with the Advanced Camera for Surveys of three young LMC clusters to characterize the phenomenon and develop a comparative scheme for its assessment in such clusters. The clusters of our sample, NGC 1983, NGC 2002 and NGC 2010, are selected on the basis of their youthfulness, and their variety in appearance, structure, stellar content, and surrounding stellar ambient. Our photometry is complete for magnitudes down to m814 ≃ 23 mag, allowing the calculation of the structural parameters of the clusters, the estimation of their ages and the determination of their stellar content. Our study shows that each cluster in our sample demonstrates stellar stratification in a quite different manner and at different degree from the others. Specifically, NGC 1983 shows to be partially segregated with the effective radius increasing with fainter magnitudes only for the faintest stars of the cluster.