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Naming the Extrasolar Planets
Naming the extrasolar planets W. Lyra Max Planck Institute for Astronomy, K¨onigstuhl 17, 69177, Heidelberg, Germany [email protected] Abstract and OGLE-TR-182 b, which does not help educators convey the message that these planets are quite similar to Jupiter. Extrasolar planets are not named and are referred to only In stark contrast, the sentence“planet Apollo is a gas giant by their assigned scientific designation. The reason given like Jupiter” is heavily - yet invisibly - coated with Coper- by the IAU to not name the planets is that it is consid- nicanism. ered impractical as planets are expected to be common. I One reason given by the IAU for not considering naming advance some reasons as to why this logic is flawed, and sug- the extrasolar planets is that it is a task deemed impractical. gest names for the 403 extrasolar planet candidates known One source is quoted as having said “if planets are found to as of Oct 2009. The names follow a scheme of association occur very frequently in the Universe, a system of individual with the constellation that the host star pertains to, and names for planets might well rapidly be found equally im- therefore are mostly drawn from Roman-Greek mythology. practicable as it is for stars, as planet discoveries progress.” Other mythologies may also be used given that a suitable 1. This leads to a second argument. It is indeed impractical association is established. to name all stars. But some stars are named nonetheless. In fact, all other classes of astronomical bodies are named. -
Guide Du Ciel Profond
Guide du ciel profond Olivier PETIT 8 mai 2004 2 Introduction hjjdfhgf ghjfghfd fg hdfjgdf gfdhfdk dfkgfd fghfkg fdkg fhdkg fkg kfghfhk Table des mati`eres I Objets par constellation 21 1 Androm`ede (And) Andromeda 23 1.1 Messier 31 (La grande Galaxie d'Androm`ede) . 25 1.2 Messier 32 . 27 1.3 Messier 110 . 29 1.4 NGC 404 . 31 1.5 NGC 752 . 33 1.6 NGC 891 . 35 1.7 NGC 7640 . 37 1.8 NGC 7662 (La boule de neige bleue) . 39 2 La Machine pneumatique (Ant) Antlia 41 2.1 NGC 2997 . 43 3 le Verseau (Aqr) Aquarius 45 3.1 Messier 2 . 47 3.2 Messier 72 . 49 3.3 Messier 73 . 51 3.4 NGC 7009 (La n¶ebuleuse Saturne) . 53 3.5 NGC 7293 (La n¶ebuleuse de l'h¶elice) . 56 3.6 NGC 7492 . 58 3.7 NGC 7606 . 60 3.8 Cederblad 211 (N¶ebuleuse de R Aquarii) . 62 4 l'Aigle (Aql) Aquila 63 4.1 NGC 6709 . 65 4.2 NGC 6741 . 67 4.3 NGC 6751 (La n¶ebuleuse de l’œil flou) . 69 4.4 NGC 6760 . 71 4.5 NGC 6781 (Le nid de l'Aigle ) . 73 TABLE DES MATIERES` 5 4.6 NGC 6790 . 75 4.7 NGC 6804 . 77 4.8 Barnard 142-143 (La tani`ere noire) . 79 5 le B¶elier (Ari) Aries 81 5.1 NGC 772 . 83 6 le Cocher (Aur) Auriga 85 6.1 Messier 36 . 87 6.2 Messier 37 . 89 6.3 Messier 38 . -
Allianz Funds Multi-Strategy Trust Form N-CSRS Filed 2017-06-02
SECURITIES AND EXCHANGE COMMISSION FORM N-CSRS Certified semi-annual shareholder report of registered management investment companies filed on Form N-CSR Filing Date: 2017-06-02 | Period of Report: 2017-03-31 SEC Accession No. 0001193125-17-192768 (HTML Version on secdatabase.com) FILER Allianz Funds Multi-Strategy Trust Mailing Address Business Address C/O ALLIANZ GLOBAL C/O ALLIANZ GLOBAL CIK:1423227| IRS No.: 000000000 | State of Incorp.:MA INVESTORS INVESTORS Type: N-CSRS | Act: 40 | File No.: 811-22167 | Film No.: 17887508 1633 BROADWAY 1633 BROADWAY NEW YORK NY 10019 NEW YORK NY 10019 212-739-3000 Copyright © 2017 www.secdatabase.com. All Rights Reserved. Please Consider the Environment Before Printing This Document Table of Contents UNITED STATES SECURITIES AND EXCHANGE COMMISSION Washington, D.C. 20549 FORM N-CSR CERTIFIED SHAREHOLDER REPORT OF REGISTERED MANAGEMENT INVESTMENT COMPANIES Investment Company Act file number: 811-22167 Allianz Funds Multi-Strategy Trust (Exact name of registrant as specified in charter) 1633 Broadway, New York, NY 10019 (Address of principal executive offices) (Zip code) Lawrence G. Altadonna 1633 Broadway, New York, NY 10019 (Name and address of agent for service) Registrants telephone number, including area code: 212-739-3371 Date of fiscal year end: September 30 Date of reporting period: March 31, 2017 Copyright © 2017 www.secdatabase.com. All Rights Reserved. Please Consider the Environment Before Printing This Document Table of Contents Item 1. Report to Shareholders Allianz Multi-Strategy Funds -
Stellar Encounters with the Oort Cloud Based on Hipparcos Data Joan Garciça-Saçnchez, 1 Robert A. Preston, Dayton L. Jones, and Paul R
THE ASTRONOMICAL JOURNAL, 117:1042È1055, 1999 February ( 1999. The American Astronomical Society. All rights reserved. Printed in U.S.A. STELLAR ENCOUNTERS WITH THE OORT CLOUD BASED ON HIPPARCOS DATA JOAN GARCI A-SA NCHEZ,1 ROBERT A. PRESTON,DAYTON L. JONES, AND PAUL R. WEISSMAN Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109 JEAN-FRANCÓ OIS LESTRADE Observatoire de Paris-Section de Meudon, Place Jules Janssen, F-92195 Meudon, Principal Cedex, France AND DAVID W. LATHAM AND ROBERT P. STEFANIK Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 Received 1998 May 15; accepted 1998 September 4 ABSTRACT We have combined Hipparcos proper-motion and parallax data for nearby stars with ground-based radial velocity measurements to Ðnd stars that may have passed (or will pass) close enough to the Sun to perturb the Oort cloud. Close stellar encounters could deÑect large numbers of comets into the inner solar system, which would increase the impact hazard at Earth. We Ðnd that the rate of close approaches by star systems (single or multiple stars) within a distance D (in parsecs) from the Sun is given by N \ 3.5D2.12 Myr~1, less than the number predicted by a simple stellar dynamics model. However, this value is clearly a lower limit because of observational incompleteness in the Hipparcos data set. One star, Gliese 710, is estimated to have a closest approach of less than 0.4 pc 1.4 Myr in the future, and several stars come within 1 pc during a ^10 Myr interval. -
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. -
Index to JRASC Volumes 61-90 (PDF)
THE ROYAL ASTRONOMICAL SOCIETY OF CANADA GENERAL INDEX to the JOURNAL 1967–1996 Volumes 61 to 90 inclusive (including the NATIONAL NEWSLETTER, NATIONAL NEWSLETTER/BULLETIN, and BULLETIN) Compiled by Beverly Miskolczi and David Turner* * Editor of the Journal 1994–2000 Layout and Production by David Lane Published by and Copyright 2002 by The Royal Astronomical Society of Canada 136 Dupont Street Toronto, Ontario, M5R 1V2 Canada www.rasc.ca — [email protected] Table of Contents Preface ....................................................................................2 Volume Number Reference ...................................................3 Subject Index Reference ........................................................4 Subject Index ..........................................................................7 Author Index ..................................................................... 121 Abstracts of Papers Presented at Annual Meetings of the National Committee for Canada of the I.A.U. (1967–1970) and Canadian Astronomical Society (1971–1996) .......................................................................168 Abstracts of Papers Presented at the Annual General Assembly of the Royal Astronomical Society of Canada (1969–1996) ...........................................................207 JRASC Index (1967-1996) Page 1 PREFACE The last cumulative Index to the Journal, published in 1971, was compiled by Ruth J. Northcott and assembled for publication by Helen Sawyer Hogg. It included all articles published in the Journal during the interval 1932–1966, Volumes 26–60. In the intervening years the Journal has undergone a variety of changes. In 1970 the National Newsletter was published along with the Journal, being bound with the regular pages of the Journal. In 1978 the National Newsletter was physically separated but still included with the Journal, and in 1989 it became simply the Newsletter/Bulletin and in 1991 the Bulletin. That continued until the eventual merger of the two publications into the new Journal in 1997. -
View & Download
78-8970 70MM REFRACTOR WITH REALVOICE™ OUTPUT INSTRUCTION MANUAL 78-8930 76MM REFLECTOR MANUEL D’INSTRUCTIONS MANUAL DE INSTRUCCIONES BEDIENUNGSANLEITUNG MANUALE DI ISTRUZIONI MANUAL DE INSTRUÇÕES 78-8945 114MM REFLECTOR Lit.#: 98-0965/06-07 PAGE GUIDE ENGLISH ............... 4 Catalog Index........... 18 FrANÇAIS.............. 34 ESPAÑOL ............... 50 DEUTSCH............... 66 ITALIANO............... 82 PORTUGUÊS........... 98 ENGLISH Congratulations on the purchase of your Bushnell Discoverer Telescope with Real Voice Output! This is one of the first telescopes ever created that actually speaks to you to educate you about the night sky. Consider this feature as your personal astronomy assistant. After reading through this manual and preparing for your observing session as outlined in these pages you can start enjoying the Real Voice Output feature by doing the following: To activate your telescope, simply turn it on! The Real Voice Output feature is built in to the remote control handset. Along the way the telescope will speak various helpful comments during the alignment process. Once aligned, the Real Voice Output feature will really shine anytime the enter key is depressed when an object name or number is displayed at the bottom right of the LCD viewscreen. That object description will be spoken to you as you follow along with the scrolling text description. If at anytime you wish to disable the speaking feature, you can cancel the speech by pressing the “Back” button on the remote control keypad. It is our sincere hope that you will enjoy this telescope for years to come! NEVER LOOK DIRECTLY AT THE SUN ❂ WITH YOUR TELESCOPE PERMANENT DAMAGE TO YOUR EYES MAY OCCUR WHERE DO I START? Your Bushnell telescope can bring the wonders of the universe to your eye. -
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. -
Legacy Image
NASA SP17069 NASA Thesaurus Astronomy Vocabulary Scientific and Technical Information Division 1988 National Aeronautics and Space Administration Washington, M= . ' NASA SP-7069 NASA Thesaurus Astronomy Vocabulary A subset of the NASA Thesaurus prepared for the international Astronomical Union Conference July 27-31,1988 This publication was prepared by the NASA Scientific and Technical Information Facility operated for the National Aeronautics and Space Administration by RMS Associates. INTRODUCTION The NASA Thesaurus Astronomy Vocabulary consists of terms used by NASA indexers as descriptors for astronomy-related documents. The terms are presented in a hierarchical format derived from the 1988 edition of the NASA Thesaurus Volume 1 -Hierarchical Listing. Main (postable) terms and non- postable cross references are listed in alphabetical order. READING THE HIERARCHY Each main term is followed by a display of its context within a hierarchy. USE references, UF (used for) references, and SN (scope notes) appear immediately below the main term, followed by GS (generic structure), the hierarchical display of term relationships. The hierarchy is headed by the broadest term within that hierarchy. Terms that are broader in meaning than the main term are listed . above the main term; terms narrower in meaning are listed below the main term. The term itself is in boldface for easy identification. Finally, a list of related terms (RT) from other hierarchies is provided. Within a hierarchy, the number of dots to the left of a term indicates its hierarchical level - the more dots, the lower the level (i.e., the narrower the meaning of the term). For example, the term "ELLIPTICAL GALAXIES" which is preceded by two dots is narrower in meaning than "GALAXIES"; this in turn is narrower than "CELESTIAL BODIES". -
Transits of Mercury, 1605–2999 CE
Appendix A Transits of Mercury, 1605–2999 CE Date (TT) Int. Offset Date (TT) Int. Offset Date (TT) Int. Offset 1605 Nov 01.84 7.0 −0.884 2065 Nov 11.84 3.5 +0.187 2542 May 17.36 9.5 −0.716 1615 May 03.42 9.5 +0.493 2078 Nov 14.57 13.0 +0.695 2545 Nov 18.57 3.5 +0.331 1618 Nov 04.57 3.5 −0.364 2085 Nov 07.57 7.0 −0.742 2558 Nov 21.31 13.0 +0.841 1628 May 05.73 9.5 −0.601 2095 May 08.88 9.5 +0.326 2565 Nov 14.31 7.0 −0.599 1631 Nov 07.31 3.5 +0.150 2098 Nov 10.31 3.5 −0.222 2575 May 15.34 9.5 +0.157 1644 Nov 09.04 13.0 +0.661 2108 May 12.18 9.5 −0.763 2578 Nov 17.04 3.5 −0.078 1651 Nov 03.04 7.0 −0.774 2111 Nov 14.04 3.5 +0.292 2588 May 17.64 9.5 −0.932 1661 May 03.70 9.5 +0.277 2124 Nov 15.77 13.0 +0.803 2591 Nov 19.77 3.5 +0.438 1664 Nov 04.77 3.5 −0.258 2131 Nov 09.77 7.0 −0.634 2604 Nov 22.51 13.0 +0.947 1674 May 07.01 9.5 −0.816 2141 May 10.16 9.5 +0.114 2608 May 13.34 3.5 +1.010 1677 Nov 07.51 3.5 +0.256 2144 Nov 11.50 3.5 −0.116 2611 Nov 16.50 3.5 −0.490 1690 Nov 10.24 13.0 +0.765 2154 May 13.46 9.5 −0.979 2621 May 16.62 9.5 −0.055 1697 Nov 03.24 7.0 −0.668 2157 Nov 14.24 3.5 +0.399 2624 Nov 18.24 3.5 +0.030 1707 May 05.98 9.5 +0.067 2170 Nov 16.97 13.0 +0.907 2637 Nov 20.97 13.0 +0.543 1710 Nov 06.97 3.5 −0.150 2174 May 08.15 3.5 +0.972 2644 Nov 13.96 7.0 −0.906 1723 Nov 09.71 13.0 +0.361 2177 Nov 09.97 3.5 −0.526 2654 May 14.61 9.5 +0.805 1736 Nov 11.44 13.0 +0.869 2187 May 11.44 9.5 −0.101 2657 Nov 16.70 3.5 −0.381 1740 May 02.96 3.5 +0.934 2190 Nov 12.70 3.5 −0.009 2667 May 17.89 9.5 −0.265 1743 Nov 05.44 3.5 −0.560 2203 Nov -
Redox DAS Artist List for Period: 01.08.2019
Page: 1 Redox D.A.S. Artist List for period: 01.08.2019 - 31.08.2019 Date time: Number: Title: Artist: Publisher Lang: 01.08.2019 00:01:22 HD 44525 I WILL LOVE YOU MONDAY (365) AURA DIONE ANG 01.08.2019 00:04:49 HD 06504 BACK FOR GOOD TAKE THAT ANG 01.08.2019 00:08:43 HD 44464 TVOJE MESTO SPI DREVORED SLO 01.08.2019 00:13:38 HD 62140 TO JE KAR IMAM GAJA PRESTOR ANG 01.08.2019 00:16:54 HD 29812 ROAM THE B 52'S ANG 01.08.2019 00:21:43 HD 55315 ALL ABOUT THAT BASS MEGHAN TRAINOR ANG 01.08.2019 00:24:50 HD 44882 DANCE, DANCE PUPPETZ SLO 01.08.2019 00:28:21 HD 04452 LOCO IN ACAPULCO FOUR TOPS ANG 01.08.2019 00:32:48 HD 00693 TELESKOP AVIA BAND SLO 01.08.2019 00:36:32 HD 33255 JUST CAN'T GET ENOUGH DEPECHE MODE ANG 01.08.2019 00:40:05 HD 29831 SING FOR ME ANDREAS JOHNSON ANG 01.08.2019 00:43:14 HD 05758 VOLIM I POSTOJIM PETAR GRASO HRV 01.08.2019 00:47:21 HD 13409 HVALA TI MALA POSODI MI JURJA SLO 01.08.2019 00:51:09 HD 63680 AMORE MIO URBAN VIDMAR SLO 01.08.2019 00:54:12 HD 06960 LOVE IS ALL AROUND WET WET WET ANG 01.08.2019 00:58:11 HD 35151 FJAKA COLONIA HRV 01.08.2019 01:00:54 HD 34411 KO BI BILO BOHEM SLO 01.08.2019 01:04:32 HD 05553 STO CON TE NEK ITA 01.08.2019 01:08:36 HD 56313 KAVA Z MLEKOM KATARINA MALA SLO 01.08.2019 01:11:52 HD 05376 GUARDIAN ANGEL MASQUERADE ANG 01.08.2019 01:16:14 HD 18905 ANOTHER CHANCE ROGER SANCHEZ ANG 01.08.2019 01:19:43 HD 53254 THE POWER CHER ANG 01.08.2019 01:23:24 HD 40565 V ISKANJU SRECE (FEAT. -
Type Shell Stars the Following Table Lists Many of the Hotter Stars
APPENDIX WILLIAM P. BID ELMAN Warner and Swasey Observatory, Case Western Reserve University, Qeveland, Ohio, U.S.A. A List of Early·Type Shell Stars The following table lists many of the hotter stars whose spectra have occasionally or continuously exhibited moderately conspicuous shell phenomena. It includes such well-known objects as P Cygni, 'Y Cassiopeiae, {3 Lyrae and R Monocerotis as well as a host of other less-studied and less-well-understood objects. Novae, classical T Tauri, VV Cephei and symbiotic stars, and stars situated outside the Galaxy have been excluded. The list is undoubtedly very incomplete: many weak or uncertain cases have been left out. It should be remembered that shell phenomena are notoriously variable in time and, in the binaries, often periodically so; thus inclusion in the list does not guarantee that an entry will exhibit shell structure at any specific time. An attempt has been made to distinguish between the objects whenever possible: category (1) includes Of stars and 0, B, and A supergiants showing P Cygni profiles; (2) includes presumably single rapidly rotating stars of classes 0, B, A and F; (3) contains stars deemed to be binary, though the shell phenomena may not always be related to this fact; and (4) is devoted to the early-type nebular objects. In many cases assignment to a particular group is very uncertain or impossible, and in the absence of fairly definite evidence to the contrary stars have generally been assigned to category (2). Many of the brighter Be stars have been found to have variable radial velocity, but they have not been considered to be binaries unless a period has been deter mined.