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121012-AAS-221 Program-14-ALL, Page 253 @ Preflight
221ST MEETING OF THE AMERICAN ASTRONOMICAL SOCIETY 6-10 January 2013 LONG BEACH, CALIFORNIA Scientific sessions will be held at the: Long Beach Convention Center 300 E. Ocean Blvd. COUNCIL.......................... 2 Long Beach, CA 90802 AAS Paper Sorters EXHIBITORS..................... 4 Aubra Anthony ATTENDEE Alan Boss SERVICES.......................... 9 Blaise Canzian Joanna Corby SCHEDULE.....................12 Rupert Croft Shantanu Desai SATURDAY.....................28 Rick Fienberg Bernhard Fleck SUNDAY..........................30 Erika Grundstrom Nimish P. Hathi MONDAY........................37 Ann Hornschemeier Suzanne H. Jacoby TUESDAY........................98 Bethany Johns Sebastien Lepine WEDNESDAY.............. 158 Katharina Lodders Kevin Marvel THURSDAY.................. 213 Karen Masters Bryan Miller AUTHOR INDEX ........ 245 Nancy Morrison Judit Ries Michael Rutkowski Allyn Smith Joe Tenn Session Numbering Key 100’s Monday 200’s Tuesday 300’s Wednesday 400’s Thursday Sessions are numbered in the Program Book by day and time. Changes after 27 November 2012 are included only in the online program materials. 1 AAS Officers & Councilors Officers Councilors President (2012-2014) (2009-2012) David J. Helfand Quest Univ. Canada Edward F. Guinan Villanova Univ. [email protected] [email protected] PAST President (2012-2013) Patricia Knezek NOAO/WIYN Observatory Debra Elmegreen Vassar College [email protected] [email protected] Robert Mathieu Univ. of Wisconsin Vice President (2009-2015) [email protected] Paula Szkody University of Washington [email protected] (2011-2014) Bruce Balick Univ. of Washington Vice-President (2010-2013) [email protected] Nicholas B. Suntzeff Texas A&M Univ. suntzeff@aas.org Eileen D. Friel Boston Univ. [email protected] Vice President (2011-2014) Edward B. Churchwell Univ. of Wisconsin Angela Speck Univ. of Missouri [email protected] [email protected] Treasurer (2011-2014) (2012-2015) Hervey (Peter) Stockman STScI Nancy S. -
Astronomy-Dyson 1910.Pdf
ASTRONOMY ^ /o A HANDY MANUAL FOR STUDENTS AND OTHERS BY F. W. DYSON, F.R.S. ASTRONOMER ROYAL FOR SCOTLAND ; PROFESSOR OF ASTRONOMY IN THE UNIVERSITY OF EDINBURGH WITH 95 DIAGRAMS AND ILLUSTRATIONS LONDON J. M. DENT & SONS, LTD. 29 & 30 BEDFORD STREET, W.C. 1910 All rights reserved PREFACE IN this little book I have attempted to give an account of the methods employed by astronomers and the reasons for some of the propositions they advance. Astronomical investigations frequently seem compli- cated owing to the amount of subsidiary detail, but the principles underlying them are simple and usually admit of a clear statement which can be followed by a general reader. In the introduction to his lectures delivered at Ipswich in 1848 Sir George Airy draws attention to an attitude towards Astronomy which is still prevalent. Such questions as the determination of the distance of the Sun or Moon are considered as the instruments with beyond ordinary comprehension ; which astronomical measurements are made are sup- to obscure difficult posed be based on and principles ; therefore the best a layman can do is to accept state- ments on the personal credit of the astronomer making them. He points out that this is an exaggerated view. The principles involved in measuring the dis- tance of the Moon are no more abstruse than those employed to find the distance of a tree on the other side of a river. Astronomical instruments are as simple in principle and far less complicated in detail than a lathe or a steam-engine. It is quite true that in both instruments and methods many subsidiary details must be attended to when great accuracy is required in order that disturbing causes may be allowed for or eliminated. -
(EU) 2018/336 of 8 March 2018 Amending Regulation
13.3.2018 EN Official Journal of the European Union L 70/1 II (Non-legislative acts) REGULATIONS COMMISSION REGULATION (EU) 2018/336 of 8 March 2018 amending Regulation (EC) No 748/2009 on the list of aircraft operators which performed an aviation activity listed in Annex I to Directive 2003/87/EC on or after 1 January 2006 specifying the administering Member State for each aircraft operator (Text with EEA relevance) THE EUROPEAN COMMISSION, Having regard to the Treaty on the Functioning of the European Union, Having regard to Directive 2003/87/EC of the European Parliament and of the Council of 13 October 2003 establishing a scheme for greenhouse gas emission allowance trading within the Community and amending Council Directive 96/61/ EC (1), and in particular Article 18a(3)(b) thereof, Whereas: (1) Directive 2008/101/EC of the European Parliament and of the Council (2) amended Directive 2003/87/EC to include aviation activities in the scheme for greenhouse gas emission allowance trading within the Union. (2) Commission Regulation (EC) No 748/2009 (3) establishes a list of aircraft operators which performed an aviation activity listed in Annex I to Directive 2003/87/EC on or after 1 January 2006. (3) That list aims to reduce the administrative burden on aircraft operators by providing information on which Member State will be regulating a particular aircraft operator. (4) The inclusion of an aircraft operator in the Union’s emissions trading scheme is dependent upon the performance of an aviation activity listed in Annex I to Directive 2003/87/EC and is not dependent on the inclusion in the list of aircraft operators established by the Commission on the basis of Article 18a(3) of that Directive. -
Macrocosmo Nº33
HA MAIS DE DOIS ANOS DIFUNDINDO A ASTRONOMIA EM LÍNGUA PORTUGUESA K Y . v HE iniacroCOsmo.com SN 1808-0731 Ano III - Edição n° 33 - Agosto de 2006 * t i •■•'• bSÈlÈWW-'^Sif J fé . ’ ' w s » ws» ■ ' v> í- < • , -N V Í ’\ * ' "fc i 1 7 í l ! - 4 'T\ i V ■ }'- ■t i' ' % r ! ■ 7 ji; ■ 'Í t, ■ ,T $ -f . 3 j i A 'A ! : 1 l 4/ í o dia que o ceu explodiu! t \ Constelação de Andrômeda - Parte II Desnudando a princesa acorrentada £ Dicas Digitais: Softwares e afins, ATM, cursos online e publicações eletrônicas revista macroCOSMO .com Ano III - Edição n° 33 - Agosto de I2006 Editorial Além da órbita de Marte está o cinturão de asteróides, uma região povoada com Redação o material que restou da formação do Sistema Solar. Longe de serem chamados como simples pedras espaciais, os asteróides são objetos rochosos e/ou metálicos, [email protected] sem atmosfera, que estão em órbita do Sol, mas são pequenos demais para serem considerados como planetas. Até agora já foram descobertos mais de 70 Diretor Editor Chefe mil asteróides, a maior parte situados no cinturão de asteróides entre as órbitas Hemerson Brandão de Marte e Júpiter. [email protected] Além desse cinturão podemos encontrar pequenos grupos de asteróides isolados chamados de Troianos que compartilham a mesma órbita de Júpiter. Existem Editora Científica também aqueles que possuem órbitas livres, como é o caso de Hidalgo, Apolo e Walkiria Schulz Ícaro. [email protected] Quando um desses asteróides cruza a nossa órbita temos as crateras de impacto. A maior cratera visível de nosso planeta é a Meteor Crater, com cerca de 1 km de Diagramadores diâmetro e 600 metros de profundidade. -
Astrophysics
Publications of the Astronomical Institute rais-mf—ii«o of the Czechoslovak Academy of Sciences Publication No. 70 EUROPEAN REGIONAL ASTRONOMY MEETING OF THE IA U Praha, Czechoslovakia August 24-29, 1987 ASTROPHYSICS Edited by PETR HARMANEC Proceedings, Vol. 1987 Publications of the Astronomical Institute of the Czechoslovak Academy of Sciences Publication No. 70 EUROPEAN REGIONAL ASTRONOMY MEETING OF THE I A U 10 Praha, Czechoslovakia August 24-29, 1987 ASTROPHYSICS Edited by PETR HARMANEC Proceedings, Vol. 5 1 987 CHIEF EDITOR OF THE PROCEEDINGS: LUBOS PEREK Astronomical Institute of the Czechoslovak Academy of Sciences 251 65 Ondrejov, Czechoslovakia TABLE OF CONTENTS Preface HI Invited discourse 3.-C. Pecker: Fran Tycho Brahe to Prague 1987: The Ever Changing Universe 3 lorlishdp on rapid variability of single, binary and Multiple stars A. Baglln: Time Scales and Physical Processes Involved (Review Paper) 13 Part 1 : Early-type stars P. Koubsfty: Evidence of Rapid Variability in Early-Type Stars (Review Paper) 25 NSV. Filtertdn, D.B. Gies, C.T. Bolton: The Incidence cf Absorption Line Profile Variability Among 33 the 0 Stars (Contributed Paper) R.K. Prinja, I.D. Howarth: Variability In the Stellar Wind of 68 Cygni - Not "Shells" or "Puffs", 39 but Streams (Contributed Paper) H. Hubert, B. Dagostlnoz, A.M. Hubert, M. Floquet: Short-Time Scale Variability In Some Be Stars 45 (Contributed Paper) G. talker, S. Yang, C. McDowall, G. Fahlman: Analysis of Nonradial Oscillations of Rapidly Rotating 49 Delta Scuti Stars (Contributed Paper) C. Sterken: The Variability of the Runaway Star S3 Arietis (Contributed Paper) S3 C. Blanco, A. -
Download This Issue (Pdf)
Volume 43 Number 1 JAAVSO 2015 The Journal of the American Association of Variable Star Observers The Curious Case of ASAS J174600-2321.3: an Eclipsing Symbiotic Nova in Outburst? Light curve of ASAS J174600-2321.3, based on EROS-2, ASAS-3, and APASS data. Also in this issue... • The Early-Spectral Type W UMa Contact Binary V444 And • The δ Scuti Pulsation Periods in KIC 5197256 • UXOR Hunting among Algol Variables • Early-Time Flux Measurements of SN 2014J Obtained with Small Robotic Telescopes: Extending the AAVSO Light Curve Complete table of contents inside... The American Association of Variable Star Observers 49 Bay State Road, Cambridge, MA 02138, USA The Journal of the American Association of Variable Star Observers Editor John R. Percy Edward F. Guinan Paula Szkody University of Toronto Villanova University University of Washington Toronto, Ontario, Canada Villanova, Pennsylvania Seattle, Washington Associate Editor John B. Hearnshaw Matthew R. Templeton Elizabeth O. Waagen University of Canterbury AAVSO Christchurch, New Zealand Production Editor Nikolaus Vogt Michael Saladyga Laszlo L. Kiss Universidad de Valparaiso Konkoly Observatory Valparaiso, Chile Budapest, Hungary Editorial Board Douglas L. Welch Geoffrey C. Clayton Katrien Kolenberg McMaster University Louisiana State University Universities of Antwerp Hamilton, Ontario, Canada Baton Rouge, Louisiana and of Leuven, Belgium and Harvard-Smithsonian Center David B. Williams Zhibin Dai for Astrophysics Whitestown, Indiana Yunnan Observatories Cambridge, Massachusetts Kunming City, Yunnan, China Thomas R. Williams Ulisse Munari Houston, Texas Kosmas Gazeas INAF/Astronomical Observatory University of Athens of Padua Lee Anne M. Willson Athens, Greece Asiago, Italy Iowa State University Ames, Iowa The Council of the American Association of Variable Star Observers 2014–2015 Director Arne A. -
Be STAR NEWSLETTER
ISSN Be STAR NEWSLETTER NUMBER September EditorinChief Technical Editor Geraldine J Peters Douglas R Gies email g jp etersmucenuscedu email giescharagsuedu Space Sciences Center Center for High Angular Resolution Astronomy University of Southern California Georgia State University University Park University Plaza Los Angeles CA Atlanta Georgia Tel Tel FAX FAX Contents Editorial Working Group Matters Working Group News Myron Smith Jir Horn and Karel Juza P Harmanec Contributions New WUPPEAstro Observations of Hot Stars K Bjorkman et al Rapid Changes in the Sp ectrum of HD W Bidelman Recent Activity in Cen O Stahl et al Observation of a V R transition in Oph R Hanuschik et al A simple and natural explanation for shell events R Hanuschik Mo de Identication for doublewave Eri Stars L Balona The Radial Velocity Variation of Eri L Balona Whats Happ ening Forthcoming Multiwavelength Campaign on Eri G Peters Intensive Campaign on Cas M Smith IUE Campaign on Ori G Peters More on Be Star h Persei J Fabregat Polarization Activity in Omicron And D McDavid Photometric Reduction Software P Harmanec Newsletters on the WWW S Cranmer NRP Movie on the WWW J Telting Preprints Received Bibliography Meetings The Be Star Newsletter is produced at and nancial ly supported by the Georgia State University -
2015 Annual Progress Report and 2016 Program Plan of the Gemini Observatory Table of Contents
2015 Annual Progress Report and 2016 Program Plan of the Gemini Observatory Table of Contents 1 Executive Summary ......................................................................................... 1 2 Introduction and Overview .............................................................................. 3 3 Science Highlights ........................................................................................... 4 3.1 The Deepest Ground-Based Photometry in a Crowded Field ...................... 4 3.2 Discovery of the Most Jupiter-like Exoplanet ............................................... 4 3.3 Best View of an Exoplanet Orbit .................................................................... 5 3.4 A Young Solar System Analog ....................................................................... 5 3.5 An Asymmetric Polarized Disk ....................................................................... 5 3.6 Water Vapor in a Terrestrial Planet Region ................................................... 6 3.7 Single-Degenerate Origin of a SNIa ............................................................... 6 3.8 Discovery of a z~6 Quasar ............................................................................. 6 3.9 Evolution of an Explosive Stellar Outflow ..................................................... 6 3.10 An Extremely Massive Black Hole at z > 6 .................................................... 7 4 Operations ....................................................................................................... -
N O T I C E This Document Has Been Reproduced From
N O T I C E THIS DOCUMENT HAS BEEN REPRODUCED FROM MICROFICHE. ALTHOUGH IT IS RECOGNIZED THAT CERTAIN PORTIONS ARE ILLEGIBLE, IT IS BEING RELEASED IN THE INTEREST OF MAKING AVAILABLE AS MUCH INFORMATION AS POSSIBLE UCLA ^ ASTRONOM& ASTROPHYSICS vi ^ a 1 ti (^ u1 Q aD w r^ r' 01 4 -+ 4 J r DEPT• ^^ s u J H O 1 U w 0tn Ub :l r^ Ow erU w vv^ ^, H 4dC «1 -z w U ^ > C ^ U \ W ^ ^ N d do ^ ^ U 7 1l1 p0 GL ^D U 1 ^1t r3 .• U 3^ 1 r. ^ w >w q EVOLUTION OF CLOSE BINARY SYSTEMS: OBSERVATIONAL ASPECTS Mirek J. Plavec Department of Astronomy University of California Las Angeles, CA 90024 Invited Review presented at the IAU Colloquium No. 69 "BINARY AND MULTIPLE STARS AS TRACERS OF STELLAR EVOLUTION" at the Remeis-Sternwarte in Bamberg, Germany in September 1981 -2- EVOLUTION OF CLOSE BINARY STARS: OBSERVATIONAL ASPECTS Mirek J. Plavec. Department of Astronomy Un'°versity of California, Los Angeles, CA 90024 ABSTRACT Detached close binary systems define the main sequence band oatis- factorily, but very little is known about the masses of giants and su- pergiants. High-dispersion IUE observations promise an improvement, since blue companions are now frequently found to late-type supergiants. The interesting cases of N Sagittarii and in particular of c Aurigae are discussed in more detail. The barium star abundance anomaly appears now to be due to mass transfer in interacting systems. The symbiotic stars are another type of binary systems containing late-type giants; several possible models for the hotter star and for the type of interaction are discussed. -
Commission Regulation (Eu) 2015
10.2.2015 EN Official Journal of the European Union L 34/1 II (Non-legislative acts) REGULATIONS COMMISSION REGULATION (EU) 2015/180 of 9 February 2015 on amending Regulation (EC) No 748/2009 on the list of aircraft operators that performed an aviation activity listed in Annex I to Directive 2003/87/EC of the European Parliament and of the Council on or after 1 January 2006 specifying the administering Member State for each aircraft operator (Text with EEA relevance) THE EUROPEAN COMMISSION, Having regard to the Treaty on the Functioning of the European Union, Having regard to Directive 2003/87/EC of the European Parliament and of the Council of 13 October 2003 establishing a scheme for greenhouse gas emission allowance trading within the Community and amending Council Directive 96/61/EC (1), and in particular Article 18a(3)(b) thereof, Whereas: (1) Directive 2008/101/EC of the European Parliament and of the Council (2) amended Directive 2003/87/EC to include aviation activities in the scheme for greenhouse gas emission allowance trading within the Union. (2) Commission Regulation (EC) No 748/2009 (3) establishes a list of aircraft operators which had performed an aviation activity as defined in Annex I to Directive 2003/87/EC on or after 1 January 2006. (3) That list aims to reduce the administrative burden on aircraft operators by providing information on which Member State will be regulating a particular aircraft operator. (4) The inclusion of an aircraft operator in the Union`s emissions trading scheme is dependent upon the performance of an aviation activity as set out in Annex I to Directive 2003/87/EC and is not dependent on the inclusion in the list of aircraft operators established by the Commission on the basis of Article 18a(3) of that Directive. -
Small Telescope Network of Korea 91 in Figure1, and the Capabilities of These Telescopes Are Pointing Based on Astrometry (Ji Et Al
Journal of the Korean Astronomical Society https://doi.org/10.5303/JKAS.2021.54.3.89 54: 89 ∼ 102, 2021 June pISSN: 1225-4614 · eISSN: 2288-890X Published under Creative Commons license CC BY-SA 4.0 http://jkas.kas.org SOMANGNET:SMALL TELESCOPE NETWORK OF KOREA Myungshin Im1,2, Yonggi Kim3,4, Chung-Uk Lee5, Hee-Won Lee6, Soojong Pak7,8, Hyunjin Shim9, Hyun-Il Sung5, Wonseok Kang10, Taewoo Kim10, Jeong-Eun Heo11, Tobias C. Hinse12, Masateru Ishiguro1,2, Gu Lim1,2, Cuc T. K. Ly´12, Gregory S. H. Paek1,2, Jinguk Seo1,2, Joh-na Yoon4, Jong-Hak Woo1,2, Hojae Ahn7, Hojin Cho1,2, Changsu Choi1,2, Jimin Han7, Sungyong Hwang1,2, Tae-Geun Ji7, Seong-Kook J. Lee1,2, Sumin Lee8, Sunwoo Lee7, Changgon Kim7, Dohoon Kim8, Joonho Kim1,2, Sophia Kim1,2, Mankeun Jeong1,2, Bomi Park1,2, Insu Paek1,2, Dohyeong Kim13, and Changbom Park14 1SNU Astronomy Research Center, Department of Physics and Astronomy, Seoul National University, Gwanak-gu, Seoul 08826, Korea; [email protected] 2Astronomy Program, Department of Physics and Astronomy, Seoul National University, Gwanak-gu, Seoul 08826, Korea 3Dept. of Astronomy & Space Science, Chungbuk National University, Chungdae-ro, Seowon-gu, Cheongju, Cheongbuk 28644, Korea 4Chungbuk National University Observatory, Eunjin-ro 29, Munbaek-Myeon, Jincheon-gun, Cheongbuk 27867, Korea 5Korea Astronomy and Space Science Institute, 776 Daedeokdae-ro, Yuseong-gu, Daejeon 34055, Korea 6Department of Astronomy and Space Science, Sejong University, 209 Neungdong-ro, Kwangjin-gu, Seoul 05006, Korea 7School of Space Research, -
FY15 High-Level Deliverables
National Optical Astronomy Observatory Fiscal Year Annual Report for FY 2015 (1 October 2014 – 30 September 2015) Submitted to the National Science Foundation Pursuant to Cooperative Support Agreement No. AST-0950945 11 December 2015 Contents NOAO MISSION PROFILE .................................................................................................... 1 1 EXECUTIVE SUMMARY ................................................................................................. 2 2 NOAO ACCOMPLISHMENTS ........................................................................................ 4 2.1 Achievements .................................................................................................... 4 2.2 Status of Vision and Goals ................................................................................ 5 2.2.1 Status of FY15 High-Level Deliverables .............................................. 5 2.2.2 FY15 Planned vs. Actual Spending and Revenues ............................... 7 2.3 Challenges and Their Impacts ......................................................................... 10 3 SCIENTIFIC ACTIVITIES AND FINDINGS ............................................................... 12 3.1 Cerro Tololo Inter-American Observatory ...................................................... 12 3.2 Kitt Peak National Observatory ....................................................................... 16 3.3 Gemini Observatory ......................................................................................... 18 4 GROUND-BASED