Communications in Asteroseismology
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Staircase of Vienna Observatory (Institut Für Astronomie Der Universität Wien)
Figure 15.1: Staircase of Vienna Observatory (Institut für Astronomie der Universität Wien) 142 15. The University Observatory Vienna Anneliese Schnell (Vienna, Austria) 15.1 Introduction should prefer non-German instrument makers (E. Weiss 1873). In spring of 2008 the new Vienna Observatory was th commemorating its 125 anniversary, it was officially During a couple of years Vienna Observatory was edit- opened by Emperor Franz Joseph in 1883. Regular ob- ing an astronomical calendar. In the 1874 edition K. L. servations had started in 1880. Viennese astronomers Littrow wrote a contribution about the new observatory had planned that observatory for a long time. Already th in which he defined the instrumental needs: Karl von Littrow’s father had plans early in the 19 “für Topographie des Himmels ein mächtiges parallakti- century (at that time according to a letter from Joseph sches Fernrohr, ein dioptrisches Instrument von 25 Zoll Johann Littrow to Gauß from December 1, 1823 the Öffnung. Da sich aber ein Werkzeug von solcher Grö- observatory of Turku was taken as model) (Reich 2008), ße für laufende Beobachtungen (Ortsbestimmung neu- but it lasted until 1867 when it was decided to build a er Planeten und Kometen, fortgesetzte Doppelsternmes- new main building of the university of Vienna and also sungen, etc.) nicht eignet, ein zweites, kleineres, daher a new observatory. Viennese astronomers at that time leichter zu handhabendes, aber zur Beobachtung licht- had an excellent training in mathematics, they mostly schwacher Objekte immer noch hinreichendes Teleskop worked on positional astronomy and celestial mechanics. von etwa 10 Zoll Öffnung, und ein Meridiankreis er- They believed in F. -
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, -
Gudrun Wolfschmidt (Hg.) Booklet of Abstracts
Gudrun Wolfschmidt (Hg.) Booklet of Abstracts Internationality in the Astronomical Research of the 18th to 20th Century Hamburg: Zentrum für Geschichte der Naturwissenschaften 2018 Gudrun Wolfschmidt (ed.) Booklet of Abstracts Tagung des Arbeitskreises Astronomiegeschichte in der Astronomischen Gesellschaft (AKAG) Internationalität in der astronomischen Forschung des 18. bis 20. Jahrhunderts Colloquium of the Working Group History of Astronomy in the Astronomical Society Internationality in the Astronomical Research of the 18th to 20th Century Wien, 17.–19. August 2018 Hamburg: Center for History of Science and Technology 2018 2 Gudrun Wolfschmidt (Hg.): AKAG Wien 2018 – Internationalität Wolfschmidt, Gudrun: Booklet of Abstracts – Internationalität in der astronomischen Forschung des 18. bis 20. Jahrhunderts – Internationality in the Astronomical Research of the 18th to 20th Century. Colloquium of the Working Group History of Astronomy in the Astronomical Society, Wien, Kuffner Sternwarte, 17.–19. August 2018. Webpage of the conference in Wien: https://www.hs.uni-hamburg.de/DE/GNT/events/akag-wien-2018.php. Cover vorn: Sonnenuntergang am Paranal mit VLT, Mond und Venus (ESO, Y. Beletsky) Cover hinten: Kuffner Sternwarte Wien bei Nacht (© Kuffner Sternwarte) Prof. Dr. Gudrun Wolfschmidt Center for History of Science and Technology Hamburg Observatory, Department of Physics, Faculty of Mathematics, Informatics and Natural Sciences Hamburg University Bundesstraße 55, Geomatikum D-20146 Hamburg Tel. +49-40-42838-5262, -9126 (-9129) Fax: +49-40-42838-9132 http://www.hs.uni-hamburg.de/DE/Ins/Per/Wolfschmidt/index.html http://www.hs.uni-hamburg.de/DE/GNT/w.htm. Inhaltsverzeichnis AKAG Wien 2018 – Internationalität in der astronomischen Forschung des 18. bis 20. Jahrhunderts 5 1.0.1 SOC – Scientific Organizing Committee . -
The Evening Sky Map
I N E D R I A C A S T N E O D I T A C L E O R N I G D S T S H A E P H M O O R C I . Z N O p l f e i n h d o P t O o N ) l h a r g Z i u s , o I l C t P h R I r e o R N ( O o r C r H e t L p h p E E i s t D H a ( r g T F i . O B NORTH D R e N M h t E A X O e s A H U M C T . I P N S L E E P Z “ E A N H O NORTHERN HEMISPHERE M T R T Y N H E ” K E η ) W S . T T E W U B R N W D E T T W T H h A The Evening Sky Map e MAY 2021 E . C ) Cluster O N FREE* EACH MONTH FOR YOU TO EXPLORE, LEARN & ENJOY THE NIGHT SKY r S L a o K e Double r Y E t B h R M t e PERSEUS A a A r CASSIOPEIA n e S SKY MAP SHOWS HOW Get Sky Calendar on Twitter P δ r T C G C A CEPHEUS r E o R e J s O h Sky Calendar – May 2021 http://twitter.com/skymaps M39 s B THE NIGHT SKY LOOKS T U ( O i N s r L D o a j A NE I I a μ p T EARLY MAY PM T 10 r 61 M S o S 3 Last Quarter Moon at 19:51 UT. -
August 2017 BRAS Newsletter
August 2017 Issue Next Meeting: Monday, August 14th at 7PM at HRPO nd (2 Mondays, Highland Road Park Observatory) Presenters: Chris Desselles, Merrill Hess, and Ben Toman will share tips, tricks and insights regarding the upcoming Solar Eclipse. What's In This Issue? President’s Message Secretary's Summary Outreach Report - FAE Light Pollution Committee Report Recent Forum Entries 20/20 Vision Campaign Messages from the HRPO Perseid Meteor Shower Partial Solar Eclipse Observing Notes – Lyra, the Lyre & Mythology Like this newsletter? See past issues back to 2009 at http://brastro.org/newsletters.html Newsletter of the Baton Rouge Astronomical Society August 2017 President’s Message August, 21, 2017. Total eclipse of the Sun. What more can I say. If you have not made plans for a road trip, you can help out at HRPO. All who are going on a road trip be prepared to share pictures and experiences at the September meeting. BRAS has lost another member, Bart Bennett, who joined BRAS after Chris Desselles gave a talk on Astrophotography to the Cajun Clickers Computer Club (CCCC) in January of 2016, Bart became the President of CCCC at the same time I became president of BRAS. The Clickers are shocked at his sudden death via heart attack. Both organizations will miss Bart. His obituary is posted online here: http://www.rabenhorst.com/obituary/sidney-barton-bart-bennett/ Last month’s meeting, at LIGO, was a success, even though there was not much solar viewing for the public due to clouds and rain for most of the afternoon. BRAS had a table inside the museum building, where Ben and Craig used material from the Night Sky Network for the public outreach. -
The MOON in the Age of PHOTOGRAPHY 1859-1969
The MOON in the Age of PHOTOGRAPHY 1859-1969 MILANEUM VINTAGE PHOTOGRAPHY The Moon in the Age of Photography 1859-1969 The photos of the moon landing on July 20, 1969 mark an important point in the history of the picture and have radically expanded the limits of human imagination. This exhibition takes place on the occasion of the 50th anniversary of the moon landing of Apollo 11. A wide range of photographs from NASA’s Apollo Program 1961 -1972, published in Austria via the U.S. Information Service (USIS), highlight #MILANEUM the culmination of technological development and international cooperation in space. (19-39) 4/2019 Photographs by the Austro-Hungarian astronomer Ladislaus Weinek from the 1880s illustrate the efforts of the 19th century to accurately depict the lunar surface. (3-6) The attraction between astronomy and photography is natural, since both are concerned with the reflectance or absorption of light upon surfaces. Around 1900 even simple studio photographers tried to profit from the fascination for the moon. (13-15) Photomontage postcards convey bizarre fantasies about life on the moon. (12/16/17) details and prices on request: [email protected] 1/2 Warren De La Rue (1815-1889) Moon, GB. ca. 1858 Stereoscopic photograph Albumine print Warren De La Rue was among the earliest astronomer-photographers and worked at Kew Observatory. De La Rue took the photos at different geographi- cal locations and different times of year. Stereophotography gives an illusion of depth. 7 3/4 Ladislaus Weinek Mondkrater (Archimedes) Lick Observatory Albumine print ca. 1888 ca. 25 x 21,5 cm 9 WEINEK, Ladislaus (*1848 in Ofen, †1913 in Prag) Weinek was educated in Vienna, and worked at the pho- 5/6 Übersicht der von Weinek in Prag 1884-1891 nach der tography laboratories in Schwerin. -
Appendix 1 1311 Discoverers in Alphabetical Order
Appendix 1 1311 Discoverers in Alphabetical Order Abe, H. 28 (8) 1993-1999 Bernstein, G. 1 1998 Abe, M. 1 (1) 1994 Bettelheim, E. 1 (1) 2000 Abraham, M. 3 (3) 1999 Bickel, W. 443 1995-2010 Aikman, G. C. L. 4 1994-1998 Biggs, J. 1 2001 Akiyama, M. 16 (10) 1989-1999 Bigourdan, G. 1 1894 Albitskij, V. A. 10 1923-1925 Billings, G. W. 6 1999 Aldering, G. 4 1982 Binzel, R. P. 3 1987-1990 Alikoski, H. 13 1938-1953 Birkle, K. 8 (8) 1989-1993 Allen, E. J. 1 2004 Birtwhistle, P. 56 2003-2009 Allen, L. 2 2004 Blasco, M. 5 (1) 1996-2000 Alu, J. 24 (13) 1987-1993 Block, A. 1 2000 Amburgey, L. L. 2 1997-2000 Boattini, A. 237 (224) 1977-2006 Andrews, A. D. 1 1965 Boehnhardt, H. 1 (1) 1993 Antal, M. 17 1971-1988 Boeker, A. 1 (1) 2002 Antolini, P. 4 (3) 1994-1996 Boeuf, M. 12 1998-2000 Antonini, P. 35 1997-1999 Boffin, H. M. J. 10 (2) 1999-2001 Aoki, M. 2 1996-1997 Bohrmann, A. 9 1936-1938 Apitzsch, R. 43 2004-2009 Boles, T. 1 2002 Arai, M. 45 (45) 1988-1991 Bonomi, R. 1 (1) 1995 Araki, H. 2 (2) 1994 Borgman, D. 1 (1) 2004 Arend, S. 51 1929-1961 B¨orngen, F. 535 (231) 1961-1995 Armstrong, C. 1 (1) 1997 Borrelly, A. 19 1866-1894 Armstrong, M. 2 (1) 1997-1998 Bourban, G. 1 (1) 2005 Asami, A. 7 1997-1999 Bourgeois, P. 1 1929 Asher, D. -
Astronomers Need Your Help!
Citizen Science with variable stars Brought to you by the AAVSO, the Naonal Science Foundaon and Your Universe Astronomers need your help! Variable stars are stars that change in brightness over 1me. There are too many for professional astronomers to monitor alone. So, we need your help to monitor these stars over days, weeks and years. This guide will help you find some bright variable stars, measure their brightness and Ci#zenSky is a collaboraon of then submit the measurements to assist the American Associaon of professional astronomers. Variable Star Observers (AAVSO), the University of Denver, the Adler Planetarium, the Johns Hopkins University Par1cipate in one of the oldest ci1zen science and the California Academies projects in history! Thousands of people just of Science with support from the Naonal Science like you are also helping out. Astronomers Foundaon. need large numbers of people to get the amount of precision they need to do their research. You are the key. Header artwork is reproduced with permission from Sky & Telescope magazine (www.skyandtelescope.com) This is a Light Curve It shows how a star’s brightness changes over 1me. Light curves are a fundamental tool for variable star astronomy. They are relavely simple and easy to grasp. They are simply a graph of brightness (Y axis) vs. 1me (X axis). Brightness increases as you go up the graph and 1me advances as you move to the right. The brightness of a star is measured in units of “magnitude”. No1ce that the magnitude scale on the graph above shows smaller numbers as the star gets brighter and larger numbers as the star gets fainter. -
THE ASTEROIDS and THEIR DISCOVERERS Rock Legends
PAUL MURDIN THE ASTEROIDS AND THEIR DISCOVERERS Rock Legends The Asteroids and Their Discoverers More information about this series at http://www.springer.com/series/4097 Paul Murdin Rock Legends The Asteroids and Their Discoverers Paul Murdin Institute of Astronomy University of Cambridge Cambridge , UK Springer Praxis Books ISBN 978-3-319-31835-6 ISBN 978-3-319-31836-3 (eBook) DOI 10.1007/978-3-319-31836-3 Library of Congress Control Number: 2016938526 © Springer International Publishing Switzerland 2016 This work is subject to copyright. All rights are reserved by the Publisher, whether the whole or part of the material is concerned, specifi cally the rights of translation, reprinting, reuse of illustrations, recitation, broadcasting, reproduction on microfi lms or in any other physical way, and transmission or information storage and retrieval, electronic adaptation, computer software, or by similar or dissimilar methodology now known or hereafter developed. The use of general descriptive names, registered names, trademarks, service marks, etc. in this publication does not imply, even in the absence of a specifi c statement, that such names are exempt from the relevant protective laws and regulations and therefore free for general use. The publisher, the authors and the editors are safe to assume that the advice and information in this book are believed to be true and accurate at the date of publication. Neither the publisher nor the authors or the editors give a warranty, express or implied, with respect to the material contained herein or for any errors or omissions that may have been made. Cover design: Frido at studio escalamar Printed on acid-free paper This Springer imprint is published by Springer Nature The registered company is Springer International Publishing AG Switzerland Acknowledgments I am grateful to Alan Fitzsimmons for taking and supplying the picture in Fig. -
August Star Parties Elections for Officers in September The
CVAS Executive Committee Pres – Dell Vance - (435) 938-8328 Loaner Scope Coordinator/NSN Coordinator – [email protected] Garrett Smith – [email protected] Vice Pres- Layne Pedersen – (801) 463-1701 Past President, Webmaster, Librarian – [email protected] Tom Westre – (435) 787-6380 [email protected] Treasurer- Brad Kropp - (435) 755-0877 Public Relations – Lyle Johnson - [email protected] Secretary – Dale Hooper - (435) 563-0608 [email protected] Vol. 5 Number 12 August 2018 www.cvas-utahskies.org No Meeting This Month – August Star September is getting closer and we want you to Parties begin thinking about running for office. There will There is no club meeting scheduled for August. be one or more open officer positions this year, so During the summer months, we instead, concentrate please consider the opportunity to run for a club on getting outside for club (private) and public star officer position. You may run for any office. parties. The President’s Corner We have three star parties scheduled for August. By Dell Vance, CVAS President Watch the website and email for changes and more information. First is a CVAS star party at the Beaver Mountain parking lot on August 10th. The next morning (11 Aug) is a solar party at the Logan Library from 10:30am to noon. The last scheduled star party is one that is always fun. We will set up scopes in the parking lot of the Providence Macey’s to show shoppers the planets and the moon. We also still need a liaison for the Logan Library Loaner Telescope. Please contact Dell Vance if you can help. -
University Microfilms, a XEROX Company, Ann Arbor, Michigan
CARBON-MONOXIDE ABSORPTION IN K AND M GIANTS AND THE CARBON-12/CARBON-13 ABUNDANCE RATIO Item Type text; Dissertation-Reproduction (electronic) Authors Bailey, Wayne Lewis, 1942- Publisher The University of Arizona. Rights Copyright © is held by the author. Digital access to this material is made possible by the University Libraries, University of Arizona. Further transmission, reproduction or presentation (such as public display or performance) of protected items is prohibited except with permission of the author. Download date 23/09/2021 15:08:21 Link to Item http://hdl.handle.net/10150/290269 71-24,887 BAILEY, Wayne Lewis, 1942- CARBON MONOXIDE ABSORPTION IN K AND M GIANTS AND THE C12/C13 ABUNDANCE RATIO. The University of Arizona, Ph.D., 1971 Astrophysics University Microfilms, A XEROX Company, Ann Arbor, Michigan THIS DISSERTATION HAS BEEN MICROFILMED EXACTLY AS RECEIVED CARBON MONOXIDE ABSORPTION IN K AND M GIANTS AND THE C12/C13 ABUNDANCE RATIO by Wayne Lewis Bailey A Dissertation Submitted to the Faculty of the DEPARTMENT OF ASTRONOMY In Partial Fulfillment of the Requirements For the Degree of DOCTOR OF PHILOSOPHY In the Graduate College THE UNIVERSITY OF ARIZONA 19 7 1 THE UNIVERSITY OF ARIZONA GRADUATE COLLEGE I hereby recommend that this dissertation prepared under my direction by Wayne Lewis Bailey entitled Carbon Monoxide Absorption in K and M Giants and the C*VC*3 Abundance Ratio be accepted as fulfilling the dissertation requirement of the degree of Doctor of Philosophy Dissertation Director f Date/7 After inspection of the final copy of the dissertation, the following members of the Final Examination Committee concur in its approval and recommend its acceptance:* P {.i/flo. -
Downloaded 4.0 License
Chapter 7 Disruption of Old Structures After a seven-month stay in Copenhagen, on May 22, 1770 Hell and Sajnovics finally left for Vienna, which they reached on August 12. The route they took was different from the outward journey. Instead of a sea voyage to Travemünde, they traveled overland in a southwestern direction, visiting first of all the Acad- emy for Nobles at Sorø, where they met the likes of Gerhard Schøning (1722– 80), a historian specializing in Norway and the ethnographic history of far northern peoples.1 Thereafter, they passed through Funen, southern Jutland, Schleswig, and Holstein to Hamburg. From Hamburg, they again chose a more westerly route, this time visiting Göttingen and Kassel before turning straight westward to Düsseldorf and then south through Cologne to Mannheim and Schwetzingen. They then headed east, via Würzburg, Ingolstadt, and Passau to reach Linz, Kremsmünster, Graz, and finally Vienna. The record of encounters with fellow astronomers or other scholars (apart from passing references to whom they met and where) is meager, but a desire to visit as many residences of Jesuit missionaries as possible, as well as observatories and other secular research institutions, appears to have been the reason behind this winding track. Hell’s grandiose dream of a long publicity tour of virtually all Western Eu- rope, as outlined in his letter to the pope before the expedition, thus did not materialize.2 Yet, he had no reason for disappointment. He and his companion were elected members of the academies of Trondheim and Copenhagen, and treated in the Danish capital as celebrities.