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The Observer's Handbook for 1912
T he O bservers H andbook FOR 1912 PUBLISHED BY THE ROYAL ASTRONOMICAL SOCIETY OF CANADA E d i t e d b y C. A, CHANT FOURTH YEAR OF PUBLICATION TORONTO 198 C o l l e g e St r e e t Pr in t e d fo r t h e So c ie t y 1912 T he Observers Handbook for 1912 PUBLISHED BY THE ROYAL ASTRONOMICAL SOCIETY OF CANADA TORONTO 198 C o l l e g e St r e e t Pr in t e d fo r t h e S o c ie t y 1912 PREFACE Some changes have been made in the Handbook this year which, it is believed, will commend themselves to observers. In previous issues the times of sunrise and sunset have been given for a small number of selected places in the standard time of each place. On account of the arbitrary correction which must be made to the mean time of any place in order to get its standard time, the tables given for a particualar place are of little use any where else, In order to remedy this the times of sunrise and sunset have been calculated for places on five different latitudes covering the populous part of Canada, (pages 10 to 21), while the way to use these tables at a large number of towns and cities is explained on pages 8 and 9. The other chief change is in the addition of fuller star maps near the end. These are on a large enough scale to locate a star or planet or comet when its right ascension and declination are given. -
September 2020 BRAS Newsletter
A Neowise Comet 2020, photo by Ralf Rohner of Skypointer Photography Monthly Meeting September 14th at 7:00 PM, via Jitsi (Monthly meetings are on 2nd Mondays at Highland Road Park Observatory, temporarily during quarantine at meet.jit.si/BRASMeets). GUEST SPEAKER: NASA Michoud Assembly Facility Director, Robert Champion What's In This Issue? President’s Message Secretary's Summary Business Meeting Minutes Outreach Report Asteroid and Comet News Light Pollution Committee Report Globe at Night Member’s Corner –My Quest For A Dark Place, by Chris Carlton Astro-Photos by BRAS Members Messages from the HRPO REMOTE DISCUSSION Solar Viewing Plus Night Mercurian Elongation Spooky Sensation Great Martian Opposition Observing Notes: Aquila – The Eagle Like this newsletter? See PAST ISSUES online back to 2009 Visit us on Facebook – Baton Rouge Astronomical Society Baton Rouge Astronomical Society Newsletter, Night Visions Page 2 of 27 September 2020 President’s Message Welcome to September. You may have noticed that this newsletter is showing up a little bit later than usual, and it’s for good reason: release of the newsletter will now happen after the monthly business meeting so that we can have a chance to keep everybody up to date on the latest information. Sometimes, this will mean the newsletter shows up a couple of days late. But, the upshot is that you’ll now be able to see what we discussed at the recent business meeting and have time to digest it before our general meeting in case you want to give some feedback. Now that we’re on the new format, business meetings (and the oft neglected Light Pollution Committee Meeting), are going to start being open to all members of the club again by simply joining up in the respective chat rooms the Wednesday before the first Monday of the month—which I encourage people to do, especially if you have some ideas you want to see the club put into action. -
Searching for Gas Emission Lines in Spitzer Infrared Spectrograph \(IRS
A&A 528, A22 (2011) Astronomy DOI: 10.1051/0004-6361/201015622 & c ESO 2011 Astrophysics Searching for gas emission lines in Spitzer Infrared Spectrograph (IRS) spectra of young stars in Taurus C. Baldovin-Saavedra1,2, M. Audard1,2, M. Güdel3,L.M.Rebull4,D.L.Padgett4, S. L. Skinner5, A. Carmona1,2,A.M.Glauser6,7, and S. B. Fajardo-Acosta8 1 ISDC Data Centre for Astrophysics, Université de Genève, 16 chemin d’Ecogia, 1290 Versoix, Switzerland e-mail: [email protected] 2 Observatoire Astronomique de l’Université de Genève, 51 chemin de Maillettes, 1290 Sauverny, Switzerland 3 University of Vienna, Department of Astronomy, Türkenschanzstrasse 17, 1180 Vienna, Austria 4 Spitzer Science Center, California Institute of Technology, 220-6 1200 East California Boulevard, CA 91125 Pasadena, USA 5 Center for Astrophysics and Space Astronomy, University of Colorado, CO 80309-0389 Boulder, USA 6 ETH Zürich, 27 Wolfgang-Pauli-Str., 8093 Zürich, Switzerland 7 UK Astronomy Technology Centre, Royal Observatory, Blackford Hill, EH3 9HJ Edinburgh, UK 8 IPAC, California Institute of Technology, 770 South Wilson Avenue, CA 91125 Pasadena, USA Received 19 August 2010 / Accepted 14 January 2011 ABSTRACT Context. Our knowledge of circumstellar disks has traditionally been based on studies of dust. However, gas dominates the disk mass and its study is key to our understanding of accretion, outflows, and ultimately planet formation. The Spitzer Space Telescope provides access to gas emission lines in the mid-infrared, providing crucial new diagnostics of the physical conditions in accretion disks and outflows. Aims. We seek to identify gas emission lines in mid-infrared spectra of 64 pre-main-sequence stars in Taurus. -
July OBSERVER(220Dpi)
THE OBSERVER OF THE TWIN CITY AMATEUR ASTRONOMERS Volume 45, Number 7 July 2020 INSIDE THIS ISSUE: 1«Editor’s Choice: Image of the Month – Messier 27 2«President’s Note 2«NCRAL’s Season Messier Mini Marathons 3«Calendar of Astronomical Events – July 2020 3«New & Renewing Members/Dues Blues/E-Mail List 4«This Month’s Phases of the Moon 4«This Month’s Solar Phenomena 4«AstroBits – News from Around the TCAA 6«Waynesville Observatory Use Policy Statement 7«CDK 24” Telescope Coming Online at WO 7«Celestron NexStar 11” Telescope Donated to TCAA 8«TCAA Image Gallery 9«Maintenance Work at Waynesville Observatory 10«Did You Know? 11«TCAA Active on Facebook 11«July 2020 with Jeffrey L. Hunt 23«Renewing Your TCAA Membership 23«Online Public Talks for 2020 24«TCAA Treasurer’s Report as of June 26, 2020 The TCAA is an affiliate of the Astronomical League as well as its North Central Region. For more information about the TCAA, be certain to visit the TCAA website at http://www.tcaa.us/ Visit http://www.astroleague.org for additional information about the Astronomical League and its EDITOR’S CHOICE: IMAGE OF THE MONTH – MESSIER 27 numerous membership benefits, including observing programs. This image of M27 (Dumbbell Nebula) was taken by Scott and Emily Wade and Deva Chatrathi. Scott writes, “Here’s an image of M27 Also, visit the NCRAL website at that was captured on the evenings of 6/23 (Emily & Scott) and 6/25 http://ncral.wordpress.com for in- (Deva & Scott) using the CDK 17” telescope with the QHY600 formation about our North Central camera and RGB filters. -
Astronomical Coordinate Systems
Appendix 1 Astronomical Coordinate Systems A basic requirement for studying the heavens is being able to determine where in the sky things are located. To specify sky positions, astronomers have developed several coordinate systems. Each sys- tem uses a coordinate grid projected on the celestial sphere, which is similar to the geographic coor- dinate system used on the surface of the Earth. The coordinate systems differ only in their choice of the fundamental plane, which divides the sky into two equal hemispheres along a great circle (the fundamental plane of the geographic system is the Earth’s equator). Each coordinate system is named for its choice of fundamental plane. The Equatorial Coordinate System The equatorial coordinate system is probably the most widely used celestial coordinate system. It is also the most closely related to the geographic coordinate system because they use the same funda- mental plane and poles. The projection of the Earth’s equator onto the celestial sphere is called the celestial equator. Similarly, projecting the geographic poles onto the celestial sphere defines the north and south celestial poles. However, there is an important difference between the equatorial and geographic coordinate sys- tems: the geographic system is fixed to the Earth and rotates as the Earth does. The Equatorial system is fixed to the stars, so it appears to rotate across the sky with the stars, but it’s really the Earth rotating under the fixed sky. The latitudinal (latitude-like) angle of the equatorial system is called declination (Dec. for short). It measures the angle of an object above or below the celestial equator. -
1949 Handbook of the British Astronomical Association
THE HANDBOOK OF THE BRITISH ASTRONOMICAL ASSOCIATION 1 9 4 9 1948 NOVEMBER Price to Members 3s. N on Members 5s. CONTENTS Preface ... ... ... ... ... ... ... 1 Planetary Diagram ... ... ... ' ... 2 V i s i b i l i t y o f P l a n e t s ....................................................................... ........................................................................ 3 Tim e Reckoning .........................! ............................ ........................................................................ 4 S u n , 1 9 4 9 ............................................................................................................................................................... 5 Eclipses, 1949 .................................................................... .. ............................_ .................................. 8 M o o n , 1 9 4 9 . ....................................................................... ............................ 9 L i b r a t i o n ............................................................................................. .................................................. 1 0 O b s e r v a t i o n o f O c c u l t a t i o n s . .................................................................................................................... 1 0 L unar O ccultations, 1949 ........................... .................................................. 1 2 A p p e a r a n c e o f P l a n e t s ................................................................... .................................................................... -
Ephemerides Astronomicae. Anni...Ad Meridianum Mediolanensem
Informazioni su questo libro Si tratta della copia digitale di un libro che per generazioni è stato conservata negli scaffali di una biblioteca prima di essere digitalizzato da Google nell’ambito del progetto volto a rendere disponibili online i libri di tutto il mondo. Ha sopravvissuto abbastanza per non essere più protetto dai diritti di copyright e diventare di pubblico dominio. Un libro di pubblico dominio è un libro che non è mai stato protetto dal copyright o i cui termini legali di copyright sono scaduti. La classificazione di un libro come di pubblico dominio può variare da paese a paese. I libri di pubblico dominio sono l’anello di congiunzione con il passato, rappresentano un patrimonio storico, culturale e di conoscenza spesso difficile da scoprire. Commenti, note e altre annotazioni a margine presenti nel volume originale compariranno in questo file, come testimonianza del lungo viaggio percorso dal libro, dall’editore originale alla biblioteca, per giungere fino a te. Linee guide per l’utilizzo Google è orgoglioso di essere il partner delle biblioteche per digitalizzare i materiali di pubblico dominio e renderli universalmente disponibili. I libri di pubblico dominio appartengono al pubblico e noi ne siamo solamente i custodi. Tuttavia questo lavoro è oneroso, pertanto, per poter continuare ad offrire questo servizio abbiamo preso alcune iniziative per impedire l’utilizzo illecito da parte di soggetti commerciali, compresa l’imposizione di restrizioni sull’invio di query automatizzate. Inoltre ti chiediamo di: + Non fare un uso commerciale di questi file Abbiamo concepito Google Ricerca Libri per l’uso da parte dei singoli utenti privati e ti chiediamo di utilizzare questi file per uso personale e non a fini commerciali. -
Aerodynamic Phenomena in Stellar Atmospheres, a Bibliography
- PB 151389 knical rlote 91c. 30 Moulder laboratories AERODYNAMIC PHENOMENA STELLAR ATMOSPHERES -A BIBLIOGRAPHY U. S. DEPARTMENT OF COMMERCE NATIONAL BUREAU OF STANDARDS ^M THE NATIONAL BUREAU OF STANDARDS Functions and Activities The functions of the National Bureau of Standards are set forth in the Act of Congress, March 3, 1901, as amended by Congress in Public Law 619, 1950. These include the development and maintenance of the national standards of measurement and the provision of means and methods for making measurements consistent with these standards; the determination of physical constants and properties of materials; the development of methods and instruments for testing materials, devices, and structures; advisory services to government agencies on scientific and technical problems; in- vention and development of devices to serve special needs of the Government; and the development of standard practices, codes, and specifications. The work includes basic and applied research, development, engineering, instrumentation, testing, evaluation, calibration services, and various consultation and information services. Research projects are also performed for other government agencies when the work relates to and supplements the basic program of the Bureau or when the Bureau's unique competence is required. The scope of activities is suggested by the listing of divisions and sections on the inside of the back cover. Publications The results of the Bureau's work take the form of either actual equipment and devices or pub- lished papers. -
Herbig-Haro Flows and the Birth of Low Mass Stars
INTERNATIONAL ASTRONOMICAL UNION SYMPOSIUM No. 182 HERBIG-HARO FLOWS AND THE BIRTH OF LOW MASS STARS Edited by BO REIPURTH AND CLAUDE BERTOUT INTERNATIONAL ASTRONOMICAL UNION KLUWER ACADEMIC PUBLISHERS Downloaded from https://www.cambridge.org/core. IP address: 170.106.34.90, on 30 Sep 2021 at 12:35:12, subject to the Cambridge Core terms of use, available at https://www.cambridge.org/core/terms. https://doi.org/10.1017/S0074180900061994 HERBIG-HARO FLOWS AND THE BIRTH OF LOW MASS STARS Downloaded from https://www.cambridge.org/core. IP address: 170.106.34.90, on 30 Sep 2021 at 12:35:12, subject to the Cambridge Core terms of use, available at https://www.cambridge.org/core/terms. https://doi.org/10.1017/S0074180900061994 INTERNATIONAL ASTRONOMICAL UNION UNION ASTRONOMIQUE INTERNATIONALE HERBIG-HARO FLOWS AND THE BIRTH OF LOW MASS STARS PROCEEDINGS OF THE 182ND SYMPOSIUM OF THE INTERNATIONAL ASTRONOMICAL UNION, HELD IN CHAMONIX, FRANCE, 20-26 JANUARY 1997 EDITED BY BO REIPURTH Observatoire de Grenoble, France and CLAUDE BERTOUT Institut d'Astrophysique de Paris, France mm KLUWER ACADEMIC PUBLISHERS DORDRECHT / BOSTON / LONDON Downloaded from https://www.cambridge.org/core. IP address: 170.106.34.90, on 30 Sep 2021 at 12:35:12, subject to the Cambridge Core terms of use, available at https://www.cambridge.org/core/terms. https://doi.org/10.1017/S0074180900061994 Library of Congress Cataloging-in-Publication Data ISBN 0-7923-4660-2 (HB) Published on behalf of the International Astronomical Union by Kluwer Academic Publishersf P.O. Box 17,3300 AA Dordrecht, The Netherlands. -
I N S I D E T H I S I S S
February / février 2008 Volume/volume 102 Number/numéro 1 [728] This Issue's Winning Astrophoto! FEATURING A FULL COLOUR SECTION! The Journal of the Royal Astronomical Society of Canada Cassiopeia Rising Over the Plaskett by Charles Banville, Victoria Centre. This is a montage of two pictures I took using a Canon 20Da and a Canon EF 17-40mm f/4L lens. The foreground image was acquired at the Dominion Astrophysical Observatory in Victoria on 2007 July 26. That evening the Plaskett Dome was illuminated by a bright 12-day-old Moon. The star trails were created using 87 light frames of 1 minute each taken from Cattle Point on 2007 August 8. Le Journal de la Société royale d’astronomie du Canada [Editor’s Note: The two-member team of Dietmar Kupke and Paul Mortfield of the Toronto Centre selected this late-entry image from among the 30 or so entries to the “Own the Back Cover” con- test. Thanks to all the submitters. We welcome further entries, so don’t delay – send in yours now! INSIDE THIS ISSUE Watch the back cover of the April issue for the next winner.] One Hundred Editions of the Observer's Handbook · Seriously Seeking Ceres! Mont-Mégantic Dark-Sky Reserve Conference, 2007 September 19-21 Duplicity of ZC1042: My First Double-Star Discovery In Memory of Gertrude Jean Southam Building for the International Year of Astronomy (IYA2009) THE ROYAL ASTRONOMICAL SOCIETY OF CANADA February / février 2008 NATIONAL OFFICERS AND COUNCIL FOR 2007-2008/CONSEIL ET ADMINISTRATEURS NATIONAUX Honorary President Robert Garrison, Ph.D., Toronto President Scott Young, B.Sc., Winnipeg Vol. -
Biological Damage of Uv Radiation in Environments Of
BIOLOGICAL DAMAGE OF UV RADIATION IN ENVIRONMENTS OF F-TYPE STARS by SATOKO SATO Presented to the Faculty of the Graduate School of The University of Texas at Arlington in Partial Fulfillment of the Requirements for the Degree of DOCTOR OF PHILOSOPHY THE UNIVERSITY OF TEXAS AT ARLINGTON May 2014 Copyright c by Satoko Sato 2014 All Rights Reserved I dedicate this to my daughter Akari Y. Sato. Acknowledgements First of all, I would like to thank my supervising professor Dr. Manfred Cuntz. His advice on my research and academic life has always been invaluable. I would have given up the Ph.D. bound program without his encouragement and generous support as the supervising professor during a few difficult times in my life. I would like to thank Dr. Wei Chen, Dr. Yue Deng, Dr. Zdzislaw E. Musielak, and Dr. Sangwook Park for their interest in my research and for their time to serve in my committee. Next, I would like to acknowledge my research collaborators at University of Guanajuato, Cecilia M. Guerra Olvera, Dr. Dennis Jack, and Dr. Klaus-Peter Schr¨oder,for providing me the data of F-type evolutionary tracks and UV spectra. I would also like to express my deep gratitude to my parents, Hideki and Kumiko Yakushigawa, for their enormous support in many ways in my entire life, and to my sister, Tomoko Yakushigawa, for her constant encouragement to me. I am grateful to my husband, Makito Sato, and my daughter, Akari Y. Sato. Their presence always gives me strength. I am thankful to my parents-in-law, Hisao and Tsuguho Sato, and my grand-parents-in-law, Kanji and Ayako Momoi, for their financial support and prayers. -
Mapping Stellar Kinematics Across the Galactic Bar: HST Measurements Of
Mon. Not. R. Astron. Soc. 000, 000–000 (2006) Printed 24 October 2018 (MN LATEX style file v2.2) Mapping stellar kinematics across the Galactic bar: HST measurements of proper motions in 35 fields. ⋆ S. Koz lowski1†, P. R. Wo´zniak2, S. Mao1, M. C. Smith3, T. Sumi4, W. T. Vestrand2 andL. Wyrzykowski5 1 Jodrell Bank Observatory, The University of Manchester, Macclesfield, Cheshire SK11 9DL, UK 2 Los Alamos National Laboratory, MS-D466, Los Alamos, NM 87545, USA 3 Kapteyn Institute, PO Box 800, 9700 AV Groningen, the Netherlands 4 Princeton University Observatory, Princeton, NJ 08544, USA 5 Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 OHA, UK Accepted 2006 April 26. Received 2006 April 26; in original form 2006 March 22 ABSTRACT We present a proper motion mini-survey of 35 fields in the vicinity of Baade window, (l,b) = (1◦, −4◦), sampling roughly a 5 × 2.5 deg region of the Galactic bar. Our second epoch observations collected with the ACS/HRC instrument on board the Hubble Space Telescope were combined with the archival WFPC2/PC images. The resulting time baselines are in the range of 4–8 years. Precise proper motions of 15,863 stars were determined in the reference frame defined by the mean motion of stars with magnitudes between IF 814W = 16.5 − 21.5 along the line of sight. We clearly detect −1 small gradients in proper motion dispersions (σl, σb) ∼ (3.0, 2.5) mas yr , and in the amount of anisotropy (σl/σb ∼ 1.2). Both the longitude dispersion σl and its ratio to the vertical motion σb increase toward the Galactic plane.