Observer's Handbook 1975
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
Constellation Is the Corona Australis
CORONA AUSTRALIS, THE SOUTHERN CROWN Corona Australis is a constellation in the southern celestial hemisphere. Its Latin name means "southern crown", and it is the southern counterpart of Corona Borealis, the northern crown. One of the 48 constellations listed by the 2nd-century astronomer Ptolemy, it remains one of the 88 modern constellations. The Ancient Greeks saw Corona Australis as a wreath rather than a crown and associated it with Sagittarius or Centaurus. Other cultures have likened the pattern to a turtle, ostrich nest, a tent, or even a hut belonging to a rock hyrax (a shrewmouse; a small, well-furred, rotund animals with short tails). Although fainter than its northern namesake, the oval - or horseshoe-shaped pattern of its brighter stars renders it distinctive. Alpha and Beta Coronae Australis are its two brightest stars with an apparent magnitude of around 4.1. Epsilon Coronae Australis is the brightest example of a W Ursae Majoris variable in the southern sky (an eclipsing contact binary). Lying alongside the Milky Way, Corona Australis contains one of the closest star-forming regions to our Solar System —a dusty dark nebula known as the Corona Australis Molecular Cloud, lying about 430 light years away. Within it are stars at the earliest stages of their lifespan. The variable stars R and TY Coronae Australis light up parts of the nebula, which varies in brightness accordingly. Corona Australis is bordered by Sagittarius to the north, Scorpius to the west, Telescopium to the south, and Ara to the southwest. The three-letter abbreviation for the constellation, as adopted by the International Astronomical Union in 1922, is 'CrA'. -
GEORGE HERBIG and Early Stellar Evolution
GEORGE HERBIG and Early Stellar Evolution Bo Reipurth Institute for Astronomy Special Publications No. 1 George Herbig in 1960 —————————————————————– GEORGE HERBIG and Early Stellar Evolution —————————————————————– Bo Reipurth Institute for Astronomy University of Hawaii at Manoa 640 North Aohoku Place Hilo, HI 96720 USA . Dedicated to Hannelore Herbig c 2016 by Bo Reipurth Version 1.0 – April 19, 2016 Cover Image: The HH 24 complex in the Lynds 1630 cloud in Orion was discov- ered by Herbig and Kuhi in 1963. This near-infrared HST image shows several collimated Herbig-Haro jets emanating from an embedded multiple system of T Tauri stars. Courtesy Space Telescope Science Institute. This book can be referenced as follows: Reipurth, B. 2016, http://ifa.hawaii.edu/SP1 i FOREWORD I first learned about George Herbig’s work when I was a teenager. I grew up in Denmark in the 1950s, a time when Europe was healing the wounds after the ravages of the Second World War. Already at the age of 7 I had fallen in love with astronomy, but information was very hard to come by in those days, so I scraped together what I could, mainly relying on the local library. At some point I was introduced to the magazine Sky and Telescope, and soon invested my pocket money in a subscription. Every month I would sit at our dining room table with a dictionary and work my way through the latest issue. In one issue I read about Herbig-Haro objects, and I was completely mesmerized that these objects could be signposts of the formation of stars, and I dreamt about some day being able to contribute to this field of study. -
{Download PDF} the New Patterns in the Sky Myths and Legends of The
THE NEW PATTERNS IN THE SKY MYTHS AND LEGENDS OF THE STARS 1ST EDITION PDF, EPUB, EBOOK Julius D Staal | 9780939923045 | | | | | The New Patterns in the Sky Myths and Legends of the Stars 1st edition PDF Book US presidential election Officials eye blockchain technology for November polls. Lloyd, Lucy 11 October Stars of Pegasus. Another ten have the same stars but different names. Volkswagen ID. Archive for History of Exact Sciences. The star pattern that makes up the Big Dipper is technically part of the aforementioned constellation Ursa Major. I was actually very disappointed with this book. I thought it was going to be a book of myths about the constellations, instead it was a book of weirdness by a single author. Retrieved 9 July Lots of intrigue and family arguments and even some underhanded goings on. To identify the constellations, most observers use star charts , which can be found online and in astronomy books. The illustrations are beautiful. GUR "The Bark". Paris It wasn't there at dusk, but would appear prominently just a few hours later. Pegasus is dominated by a roughly square asterism, although one of the stars, Delta Pegasi or Sirrah, is now officially considered to be Alpha Andromedae , part of Andromeda , and is more usually called "Alpheratz". However, the numerous Sumerian names in these catalogues suggest that they built on older, but otherwise unattested, Sumerian traditions of the Early Bronze Age. They also created stories to go along with these star patterns, which became the basis for many of the myths that have passed through centuries by the Greeks, Romans, Polynesians, Indigenous Americans, and members of various African tribes and Asian cultures. -
Isolierte Neutronensterne Und Ihre Sub-Stellaren Begleiter
Isolierte Neutronensterne und ihre sub-stellaren Begleiter Dissertation zur Erlangung des akademischen Grades doctor rerum naturalium (Dr. rer. nat.) vorgelegt dem Rat der Physikalisch-Astronomischen Fakult¨at der Friedrich - Schiller - Universit¨at Jena von Dipl.-Phys. Bettina Posselt geboren am 7. Juni 1977 in Bernburg Gutachter: 1. Prof. Dr. Ralph Neuh¨auser, Friedrich-Schiller-Universit¨at Jena 2. Prof. Dr. Gunther¨ Hasinger, Max-Planck-Institut fur¨ extraterrestrische Physik Garching 3. Prof. Dr. Klaus Werner, Eberhard-Karls Universit¨at Tubingen¨ Tag der letzten Rigorosumsprufung:¨ 1.12.2006 Tag der ¨offentlichen Verteidigung: 21.12.2006 Zusammenfassung Neben den Radiopulsaren, die die Mehrheit der gegenw¨artig beobachteten Neutronenster- ne ausmachen, gibt es radioleise junge Neutronensterne mit rein thermischer R¨ontgenstrahlung. Diese Neutronensterne haben ihr Emissionsmaximum unterhalb von 1 keV, sind also weiche R¨ontgenquellen. Diese Gruppe ist sehr interessant fur¨ die Forschung, weil man bei ihnen direkt die Emission der Neutronensternphotosph¨are beobachtet im Gegensatz zur magnetosph¨arischen Emission, die z.B. bei nahezu allen bekannten Radiopulsaren uberwiegt.¨ Man kennt nur sieben, vermutlich sehr nahe (< 500 pc) gelegene Vertreter die- ser Neutronensterne. Innerhalb der nahen Sonnenumgebung repr¨asentieren diese Objekte jedoch etwa ein Viertel der bekannten Neutronensternpopulation. Es stellt sich die Frage, wo und wieviel weitere, ¨ahnliche Neutronensterne auffindbar sind. Die vorliegende Arbeit widmet sich zum einen -
The COLOUR of CREATION Observing and Astrophotography Targets “At a Glance” Guide
The COLOUR of CREATION observing and astrophotography targets “at a glance” guide. (Naked eye, binoculars, small and “monster” scopes) Dear fellow amateur astronomer. Please note - this is a work in progress – compiled from several sources - and undoubtedly WILL contain inaccuracies. It would therefor be HIGHLY appreciated if readers would be so kind as to forward ANY corrections and/ or additions (as the document is still obviously incomplete) to: [email protected]. The document will be updated/ revised/ expanded* on a regular basis, replacing the existing document on the ASSA Pretoria website, as well as on the website: coloursofcreation.co.za . This is by no means intended to be a complete nor an exhaustive listing, but rather an “at a glance guide” (2nd column), that will hopefully assist in choosing or eliminating certain objects in a specific constellation for further research, to determine suitability for observation or astrophotography. There is NO copy right - download at will. Warm regards. JohanM. *Edition 1: June 2016 (“Pre-Karoo Star Party version”). “To me, one of the wonders and lures of astronomy is observing a galaxy… realizing you are detecting ancient photons, emitted by billions of stars, reduced to a magnitude below naked eye detection…lying at a distance beyond comprehension...” ASSA 100. (Auke Slotegraaf). Messier objects. Apparent size: degrees, arc minutes, arc seconds. Interesting info. AKA’s. Emphasis, correction. Coordinates, location. Stars, star groups, etc. Variable stars. Double stars. (Only a small number included. “Colourful Ds. descriptions” taken from the book by Sissy Haas). Carbon star. C Asterisma. (Including many “Streicher” objects, taken from Asterism. -
Annual Report / Rapport Annuel / Jahresbericht 1998
Annual Report / Rapport annuel / Jahresbericht 1998 EUROPEAN SOUTHERN OBSERVATORY COVER COUVERTURE UMSCHLAG Impressive images were obtained soon after Des images impressionnantes ont été reçues Beeindruckende Aufnahmen wurden ge- the multi-mode VLT Infrared Spectrometer peu de temps après l’installation de l’ins- macht kurz nachdem im November 1998 And Array Camera (ISAAC) instrument trument multi-mode ISAAC (« Infrared das Multimodus-Instrument ISAAC („Infra- was mounted at the first VLT 8.2-m Unit Spectrometer And Array Camera») au pre- red Spektrometer And Array Camera“) am mier télescope VLT de 8,2 mètres (UT1) en Telescope (UT1) in November 1998. This ersten der VLT-Teleskope (UT1) installiert colour composite image of the RCW38 star- novembre 1998. Cette image couleur com- worden war. Diese Farbaufnahme des forming complex combines Z (0.95 µm), H posite du complexe de formation stellaire (1.65 µm) and Ks (2.16 µm) exposures of a RCW38 combine des images prises en Z Sternentstehungsgebiets RCW38 ist zusam- few minutes each. Stars which have recent- (0,95 µm), H (1,65 µm) et Ks (2,16 µm), mengesetzt aus Einzelaufnahmen in Z (0,95 ly formed in clouds of gas and dust in this ayant un temps d’exposition de quelques µm), H (1,65 µm) und Ks (2,16 µm) von je region 5000 light-years away are still heav- minutes chacune. Les étoiles, récemment einigen Minuten Belichtungszeit. Die vor ily obscured and cannot be seen at optical formées dans les nuages de gaz et de pous- kurzem in den Gas- und Staubwolken dieser wavelengths but become visible at infrared sières dans cette région éloignée de 5000 5000 Lichtjahre entfernten Gegend ent- wavelengths where the obscuration is sub- années-lumière, sont extrêmement enfouies standenen Sterne sind immer noch stark stantially lower. -
Index of Astronomical Objects
Index of Astronomical Objects Constellations M33, 746, 747 Aquila, 115, 433, 488 M51 (NGC 5194), 26, 737, 752, 755 Auriga, 11 M82, 753 Chamaeleon, 103 NGC 185, 747, 748 Crux, 119 NGC 1300, 760 Cygnus, 509, 545, 547 NGC 1569, 750 Lupus, 101 NGC 4111, 739 Monoceros, 63, 104 NGC 4472, 736 Orion, 2 Small Magellanic Cloud, 746, 747 Perseus, 495 Taurus, 10 HII Regions λ Orionis, 668 Embedded Clusters 30 Doradus (Tarantula Nebula), 97, 417, 745, ρ Ophiuchi, 94, 98, 106, 411, 415 750, 758, 764 30 Doradus, 97 G192.16−3.82, 544 Arches Cluster, 734 G29.96−0.02, 534 Central Cluster, 734 G34.26+0.15, 531 IC 348, 91, 98, 109, 447 G43.18−0.52, 531 Kleinman-Low (KL) Nebula, 10, 138, 226, G5.89−0.39, 530 229, 233, 237, 455, 508, 513, 535 M8 (Lagoon Nebula), 686 NGC 2023, 96 M16 (Eagle Nebula), 126, 528, 555 NGC 2024, 96 NGC 1999, 428 NGC 2068, 96 NGC 3603, 97, 417 NGC 2071, 96 NGC 6334F, 493, 496, 512, 531 NGC 2244, 63, 67, 109, 385 NGC 7538, 97, 454 NGC 2264, 104, 107, 109, 121, 363, 686 Orion Bar, 7, 523 NGC 3603, 97, 689 Orion Nebula (M42, NGC 1976), 7, 37, 38, NGC 7538, 97 496, 552, 555 Quintuplet Cluster, 734 Rosette Nebula, 63, 556 R136, 417, 745, 750 S106, 547 S106, 96, 121, 257 S199, 560 S255 / S257, 96 S254 / S255 / S257, 96 S88B, 525 Galaxies W3(OH), 492, 507, 513 Arp 220, 753, 754, 770 W49, 115, 488, 491, 493, 512, 513 Arp 244 (The Antennae), 755 W49N, 488, 507, 509, 514, 515 Large Magellanic Cloud, 97, 417, 736, 744, W75N, 257, 509 747 VLA 1, 509 Leo I, 747 VLA 2, 509 M31 (Andromeda Galaxy), 746, 747, 749 VLA 3, 509 836 Index of Astronomical -
Deep-Sky Companions: Southern Gems Stephen James O’Meara Index More Information
Cambridge University Press 978-1-107-01501-2 - Deep-Sky Companions: Southern Gems Stephen James O’Meara Index More information Index 47 Tucanae, see clusters, globular black holes, 38, 99, 111, 203, 223, 234, cicadas, 261–262 (NGC 104) 239–240, 253, 347 Claria, J. J., 199 Abbott, Francis, 191 IC 10 X-1, 29 Clark, Tom, 191 active galactic nucleus (AGN), 99, NGC 300 X-1, 29 Clerke, Agnes, 17, 372 111, 118, 203 Blanton, Elizabeth, 99 clusters, globular Akkadians, 287 Blow, Graham, 191 core-collapse, 368, 389 Al-Sufi, 58 Blue, see nebulae, planetary (NGC disk vs. halo, 365 Alberts, Stacey, 128 3918) IC 4499, 305 Alcaino, G., 284 blue stragglers, 121, 164, 264, 305, M2, 32, 361 Alighieri, Dante, 226 336, 347, 411, 416 M3, 386 Allen, Richard Hinkley, 41, 121, Bok, Bart, 192, 374 M4, 358, 411 226, 290 Bok, Priscilla, 192 M13, 123, 131, 276, 440 Almagest, 244, 353 Bond, George Phillips, 238, 430 M15, 368, 400 Ames, Adelaide, 238 Brisbane observatory, 443 M22, see NGC 6656 Anderson, David, 58 Brisbaine, Sir Thomas, 443 M30, 368, 376 Anderson, J., 336 Bronberg Observatory, 106 M54, see NGC 6715 Anglo-Australian Telescope, 125 Bruntt, H., 312 M55, see NGC 6809 Australia Telescope Compact Bulwer-Lytton, Edward Robert, 225 M67, 339 Array, 413 Burnham Jr., Robert, 138, 228, 231, M69, see NGC 6637 Ara OB1 association, 318 322, 324, 353, 388, 398 M71, 135, 136 Aratos, 287 Buta, Ronald, 82 M79, 131 Archinal, Brent, 138, 157, 183, 219, Butterfly, see clusters, open (NGC 6405) NGC 104 (Southern Gem 2), 16–22, 231, 292, 302, 319, 328 Byrne, P. -
July 2018 BRAS Newsletter
Monthly Meeting Monday, July 9th at 7PM at HRPO (Monthly meetings are on 2nd Mondays, Highland Road Park Observatory). Presenter: J. Robert Parks, LSU Astronomy Instructor will talk about his research to characterize young stellar objects. What's In This Issue? President’s Message Secretary's Summary Outreach Report Astrophotography Group Light Pollution Committee Report “Free The Milky Way” Campaign Recent Forum Entries Messages from the HRPO Friday Night Lecture Series Edge Of Night Globe at Night Mercurian Elongation Great Martian Opposition Observing Notes – Corona Australis – The Southern Crown & Mythology Like this newsletter? See PAST ISSUES online back to 2009 Visit us on Facebook – Baton Rouge Astronomical Society Newsletter of the Baton Rouge Astronomical Society July 2018 © 2018 President’s Message We are now into summer and getting longer nights. The highlights June was the Opposition of Saturn. In space exploration news the Japan Aerospace Exploration Agency (JAXA) space probe Hayabusa2 has been sending back striking images of the asteroid (162173) Ryugu. Hayabusa2 is on a mission to return a sample to Earth in 2020. On June 30th we had the 1st Asteroid Day at HRPO . Our Secretary Krista Dison has resigned. I would like to take this moment thank her for her service. Any member willing to fill the role of Secretary should let me know. Here’s our new Member Pin. Have you claimed yours yet? REMINDERS: The BRAS Business Meeting will be Tuesday July 3 (because the 4th is a holiday), and the BRAS Monthly Meeting will be Monday July 9, both will be at HRPO and at 7 PM.