OCTOBER 2013 OT H E D Ebn V E R S E R V EOCTOBERR 2013
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Planetary Nebulae
Planetary Nebulae A planetary nebula is a kind of emission nebula consisting of an expanding, glowing shell of ionized gas ejected from old red giant stars late in their lives. The term "planetary nebula" is a misnomer that originated in the 1780s with astronomer William Herschel because when viewed through his telescope, these objects appeared to him to resemble the rounded shapes of planets. Herschel's name for these objects was popularly adopted and has not been changed. They are a relatively short-lived phenomenon, lasting a few tens of thousands of years, compared to a typical stellar lifetime of several billion years. The mechanism for formation of most planetary nebulae is thought to be the following: at the end of the star's life, during the red giant phase, the outer layers of the star are expelled by strong stellar winds. Eventually, after most of the red giant's atmosphere is dissipated, the exposed hot, luminous core emits ultraviolet radiation to ionize the ejected outer layers of the star. Absorbed ultraviolet light energizes the shell of nebulous gas around the central star, appearing as a bright colored planetary nebula at several discrete visible wavelengths. Planetary nebulae may play a crucial role in the chemical evolution of the Milky Way, returning material to the interstellar medium from stars where elements, the products of nucleosynthesis (such as carbon, nitrogen, oxygen and neon), have been created. Planetary nebulae are also observed in more distant galaxies, yielding useful information about their chemical abundances. In recent years, Hubble Space Telescope images have revealed many planetary nebulae to have extremely complex and varied morphologies. -
SEPTEMBER 2014 OT H E D Ebn V E R S E R V ESEPTEMBERR 2014
THE DENVER OBSERVER SEPTEMBER 2014 OT h e D eBn v e r S E R V ESEPTEMBERR 2014 FROM THE INSIDE LOOKING OUT Calendar Taken on July 25th in San Luis State Park near the Great Sand Dunes in Colorado, Jeff made this image of the Milky Way during an overnight camping stop on the way to Santa Fe, NM. It was taken with a Canon 2............................. First quarter moon 60D camera, an EFS 15-85 lens, using an iOptron SkyTracker. It is a single frame, with no stacking or dark/ 8.......................................... Full moon bias frames, at ISO 1600 for two minutes. Visible in this south-facing photograph is Sagittarius, and the 14............ Aldebaran 1.4˚ south of moon Dark Horse Nebula inside of the Milky Way. He processed the image in Adobe Lightroom. Image © Jeff Tropeano 15............................ Last quarter moon 22........................... Autumnal Equinox 24........................................ New moon Inside the Observer SEPTEMBER SKIES by Dennis Cochran ygnus the Swan dives onto center stage this other famous deep-sky object is the Veil Nebula, President’s Message....................... 2 C month, almost overhead. Leading the descent also known as the Cygnus Loop, a supernova rem- is the nose of the swan, the star known as nant so large that its separate arcs were known Society Directory.......................... 2 Albireo, a beautiful multi-colored double. One and named before it was found to be one wide Schedule of Events......................... 2 wonders if Albireo has any planets from which to wisp that came out of a single star. The Veil is see the pair up-close. -
Ghost Hunt Challenge 2020
Virtual Ghost Hunt Challenge 10/21 /2020 (Sorry we can meet in person this year or give out awards but try doing this challenge on your own.) Participant’s Name _________________________ Categories for the competition: Manual Telescope Electronically Aided Telescope Binocular Astrophotography (best photo) (if you expect to compete in more than one category please fill-out a sheet for each) ** There are four objects on this list that may be beyond the reach of beginning astronomers or basic telescopes. Therefore, we have marked these objects with an * and provided alternate replacements for you just below the designated entry. We will use the primary objects to break a tie if that’s needed. Page 1 TAS Ghost Hunt Challenge - Page 2 Time # Designation Type Con. RA Dec. Mag. Size Common Name Observed Facing West – 7:30 8:30 p.m. 1 M17 EN Sgr 18h21’ -16˚11’ 6.0 40’x30’ Omega Nebula 2 M16 EN Ser 18h19’ -13˚47 6.0 17’ by 14’ Ghost Puppet Nebula 3 M10 GC Oph 16h58’ -04˚08’ 6.6 20’ 4 M12 GC Oph 16h48’ -01˚59’ 6.7 16’ 5 M51 Gal CVn 13h30’ 47h05’’ 8.0 13.8’x11.8’ Whirlpool Facing West - 8:30 – 9:00 p.m. 6 M101 GAL UMa 14h03’ 54˚15’ 7.9 24x22.9’ 7 NGC 6572 PN Oph 18h12’ 06˚51’ 7.3 16”x13” Emerald Eye 8 NGC 6426 GC Oph 17h46’ 03˚10’ 11.0 4.2’ 9 NGC 6633 OC Oph 18h28’ 06˚31’ 4.6 20’ Tweedledum 10 IC 4756 OC Ser 18h40’ 05˚28” 4.6 39’ Tweedledee 11 M26 OC Sct 18h46’ -09˚22’ 8.0 7.0’ 12 NGC 6712 GC Sct 18h54’ -08˚41’ 8.1 9.8’ 13 M13 GC Her 16h42’ 36˚25’ 5.8 20’ Great Hercules Cluster 14 NGC 6709 OC Aql 18h52’ 10˚21’ 6.7 14’ Flying Unicorn 15 M71 GC Sge 19h55’ 18˚50’ 8.2 7’ 16 M27 PN Vul 20h00’ 22˚43’ 7.3 8’x6’ Dumbbell Nebula 17 M56 GC Lyr 19h17’ 30˚13 8.3 9’ 18 M57 PN Lyr 18h54’ 33˚03’ 8.8 1.4’x1.1’ Ring Nebula 19 M92 GC Her 17h18’ 43˚07’ 6.44 14’ 20 M72 GC Aqr 20h54’ -12˚32’ 9.2 6’ Facing West - 9 – 10 p.m. -
Für Astronomie Nr
für Astronomie Nr. 28 Zeitschrift der Vereinigung der Sternfreunde e.V. / VdS DAS WELTALL Orionnebel DU LEBST DARIN – ENTDECKE ES! Computerastronomie Internationales Jahr der Astronomie INTERNATIONALES ISSN 1615 - 0880 www.vds-astro.de I/ 2009 ASTRONOMIEJAHR [email protected] • www.astro-shop.com Tel.: 040/5114348 • Fax: 040/5114594 Eiffestr. 426 • 20537 Hamburg Astroart 4.0 The Night Sky Observer´s Guide Photoshop Astronomy Die aktuellste Version Dieses hilfreiche Werk Der Autor arbeitet seit fast 10 Jahren mit Photo- des bekannten Bildbe- dient der erfolg- shop, um seine Astrofotos zu bearbeiten. Die arbeitungspro- reichen Vorbereitung dabei gemachten Erfahrungen hat er in diesem grammes gibt es jetzt einer abwechslungs- speziell auf die Bedürfnisse des Amateurastro- mit interessanten reichen Deep-Sky- nomen zugeschnitte- neuen Funktionen. Nacht. Sortiert nach nen Buch gesammelt. Moderne Dateifor- Sternbildern des Die behandelten The- men sind unter ande- mate wie DSLR-RAW Sommer- und Win- rem: die technische werden unterstützt, terhimmels nden Ausstattung, Farbma- Bilder können sich detaillierte NEU nagement, Histo- durch automa- Beschreibungen Südhimmel gramme, Maskie- 3. Band tische Sternfelderken- zu hunderten rungstechniken, nung direkt überlagert werden, was die Bild- Galaxien, Nebeln, Oenen Stern- und Addition mehrerer feldrotation vernachlässigbar macht. Auch die Kugelhaufen. Der Teleskopanblick jedes Bilder, Korrektur von Bearbeitung von Farbbildern wurde erweitert. Objekts ist beschrieben und mit einem Hin- Vignettierungen, Besonderes Augenmerk liegt auf der Erken- weis bezüglich der verwendeten Optik verse- Farbhalos, Deformationen oder nung und Behandlung von Pixelfehlern der hen. 2 Bände mit insgesamt 446 Fotos, 827 überbelichteten Sternen, LRGB und vieles Aufnahme-Chips. Zeichnungen, 143 Tabellen und 431 Sternkar- mehr. Auf der beigefügten DVD benden sich 90 alle im Buch besprochenen und verwendeten Update ten. -
The Agb Newsletter
THE AGB NEWSLETTER An electronic publication dedicated to Asymptotic Giant Branch stars and related phenomena Official publication of the IAU Working Group on Abundances in Red Giants No. 165 — 1 April 2011 http://www.astro.keele.ac.uk/AGBnews Editors: Jacco van Loon and Albert Zijlstra Editorial Dear Colleagues, It is our pleasure to present you the 165th issue of the AGB Newsletter. Lots of nucleosynthesis work, pulsating stars, binaries, and AGB stars in stellar systems from globulars and the Bulge to Local Group galaxies and farther afield. Congratulations to Val´erio Ribeiro, who has just obtained his Philospher’s Degree. It’s great then to see that there are opportunitites for postdoctoral research, such as the one advertised by the group in Uppsala. Don’t miss the announcement of the very interesting workshop in wonderful Warsaw this Summer. Stefan Uttenthaler, back in Vienna, offered the following reaction to last month’s Food for Thought: ”Certainly, the PN population will not be fully representative of the underlying AGB population. Most likely not every AGB star will evolve into a PN, and also the binarity properties (incl. planets) of the population will have an impact on the evolution from the AGB to the PN phase. In fact, just in the previous issue of the Newsletter, De Marco & Soker note that the presence of a companion will alter the PN life time, and that only one quarter of all AGB stars will make a PN. Now concerning the Bulge my opinion is that in the absence of evidence that the PNe are not representative for the underlying AGB population (i.e. -
A New Radio Spectral Line Survey of Planetary Nebulae: Exploring Radiatively Driven Heating and Chemistry of Molecular Gas
Rochester Institute of Technology RIT Scholar Works Theses 12-18-2017 A New Radio Spectral Line Survey of Planetary Nebulae: Exploring Radiatively Driven Heating and Chemistry of Molecular Gas Jesse Bublitz [email protected] Follow this and additional works at: https://scholarworks.rit.edu/theses Recommended Citation Bublitz, Jesse, "A New Radio Spectral Line Survey of Planetary Nebulae: Exploring Radiatively Driven Heating and Chemistry of Molecular Gas" (2017). Thesis. Rochester Institute of Technology. Accessed from This Thesis is brought to you for free and open access by RIT Scholar Works. It has been accepted for inclusion in Theses by an authorized administrator of RIT Scholar Works. For more information, please contact [email protected]. A New Radio Spectral Line Survey of Planetary Nebulae: Exploring Radiatively Driven Heating and Chemistry of Molecular Gas Jesse Bublitz AThesisSubmittedinPartialFulfillmentofthe Requirements for the Degree of Master of Science in in Astrophysical Sciences & Technology School of Physics and Astronomy College of Science Rochester Institute of Technology Rochester, NY December 18, 2017 Abstract Planetary nebulae contain shells of cold gas and dust whose heating and chemistry is likely driven by UV and X-ray emission from their central stars and from wind-collision-generated shocks. We present the results of a survey of molecular line emissions in the 88 - 235 GHz range from nine nearby (<1.5 kpc) planetary nebulae using the 30 m telescope at the Insti- tut de Radioastronomie Millim´etrique. Rotational transitions of nine molecules, including the well-studied CO isotopologues and chemically important trace species, were observed and the results compared with and augmented by previous studies of molecular gas in PNe. -
Ciel Extrême #17 À Lire (Pdf De 6.1Mo)
ÉDITORIAL N’hésitez pas à continuer d’envoyer vos observations et surtout vos articles qui Tout d’abord, merci d’avoir renouvelé, constituent l’essentiel de CE. A bientôt au cette année encore, votre confiance en Ciel RAP pour ceux qui feront le déplacement (ô Extrême et ainsi témoigné de votre intérêt combien valable !). pour le ciel profond et l’astronomie amateur de terrain. Merci particulièrement aux géné- reux donateurs: la possibilité ne figurait pas sur le bulletin d’abonnement, mais cela n’a pas empêché deux lecteurs de donner davan- Bon ciel, tage que le prix de l’abonnement. Tant mieux pour les finances de la publication qui se portent bien comme en témoigne les comptes couverture: M 64 - B. Laville (13) 1999 joints à cet envoi. SC ø254mm, F/10, 185x; P=1.5, T=2, S=4, H=60°; Chabottes (05), alt.1000m; 09/04/99, 01h51TU; Vous trouverez également avec ce numé- 1mm=0.12’ ro un petit questionnaire (sans obligation de M 64 (NGC 4826), Com, 12h56.7m, +21°41’, s7/u149/m676; GX (R)SA(rs)ab II-III, 9.2’x4.6’, réponse) destiné à prendre la température Mv=8.5, Bs=12.4, PA115° de vos desideratas vis-à-vis du contenant et du contenu, si des possibilités d’évolution étaient envisageables dans un avenir proche. Les lecteurs ayant un e-mail recevront di- rectement sur leur boîte aux lettres ce questionnaire qu’ils pourront renvoyer faci- lement. L’anonymat sera bien sûr respecté. Merci d’avance de donner votre avis sur les sujets abordés. -
Catalogue of Excitation Classes P for 750 Galactic Planetary Nebulae
Catalogue of Excitation Classes p for 750 Galactic Planetary Nebulae Name p Name p Name p Name p NeC 40 1 Nee 6072 9 NeC 6881 10 IC 4663 11 NeC 246 12+ Nee 6153 3 NeC 6884 7 IC 4673 10 NeC 650-1 10 Nee 6210 4 NeC 6886 9 IC 4699 9 NeC 1360 12 Nee 6302 10 Nee 6891 4 IC 4732 5 NeC 1501 10 Nee 6309 10 NeC 6894 10 IC 4776 2 NeC 1514 8 NeC 6326 9 Nee 6905 11 IC 4846 3 NeC 1535 8 Nee 6337 11 Nee 7008 11 IC 4997 8 NeC 2022 12 Nee 6369 4 NeC 7009 7 IC 5117 6 NeC 2242 12+ NeC 6439 8 NeC 7026 9 IC 5148-50 6 NeC 2346 9 NeC 6445 10 Nee 7027 11 IC 5217 6 NeC 2371-2 12 Nee 6537 11 Nee 7048 11 Al 1 NeC 2392 10 NeC 6543 5 Nee 7094 12 A2 10 NeC 2438 10 NeC 6563 8 NeC 7139 9 A4 10 NeC 2440 10 NeC 6565 7 NeC 7293 7 A 12 4 NeC 2452 10 NeC 6567 4 Nee 7354 10 A 15 12+ NeC 2610 12 NeC 6572 7 NeC 7662 10 A 20 12+ NeC 2792 11 NeC 6578 2 Ie 289 12 A 21 1 NeC 2818 11 NeC 6620 8 IC 351 10 A 23 4 NeC 2867 9 NeC 6629 5 Ie 418 1 A 24 1 NeC 2899 10 Nee 6644 7 IC 972 10 A 30 12+ NeC 3132 9 NeC 6720 10 IC 1295 10 A 33 11 NeC 3195 9 NeC 6741 9 IC 1297 9 A 35 1 NeC 3211 10 NeC 6751 9 Ie 1454 10 A 36 12+ NeC 3242 9 Nee 6765 10 IC1747 9 A 40 2 NeC 3587 8 NeC 6772 9 IC 2003 10 A 41 1 NeC 3699 9 NeC 6778 9 IC 2149 2 A 43 2 NeC 3918 9 NeC 6781 8 IC 2165 10 A 46 2 NeC 4071 11 NeC 6790 4 IC 2448 9 A 49 4 NeC 4361 12+ NeC 6803 5 IC 2501 3 A 50 10 NeC 5189 10 NeC 6804 12 IC 2553 8 A 51 12 NeC 5307 9 NeC 6807 4 IC 2621 9 A 54 12 NeC 5315 2 NeC 6818 10 Ie 3568 3 A 55 4 NeC 5873 10 NeC 6826 11 Ie 4191 6 A 57 3 NeC 5882 6 NeC 6833 2 Ie 4406 4 A 60 2 NeC 5879 12 NeC 6842 2 IC 4593 6 A -
7.5 X 11.5.Threelines.P65
Cambridge University Press 978-0-521-19267-5 - Observing and Cataloguing Nebulae and Star Clusters: From Herschel to Dreyer’s New General Catalogue Wolfgang Steinicke Index More information Name index The dates of birth and death, if available, for all 545 people (astronomers, telescope makers etc.) listed here are given. The data are mainly taken from the standard work Biographischer Index der Astronomie (Dick, Brüggenthies 2005). Some information has been added by the author (this especially concerns living twentieth-century astronomers). Members of the families of Dreyer, Lord Rosse and other astronomers (as mentioned in the text) are not listed. For obituaries see the references; compare also the compilations presented by Newcomb–Engelmann (Kempf 1911), Mädler (1873), Bode (1813) and Rudolf Wolf (1890). Markings: bold = portrait; underline = short biography. Abbe, Cleveland (1838–1916), 222–23, As-Sufi, Abd-al-Rahman (903–986), 164, 183, 229, 256, 271, 295, 338–42, 466 15–16, 167, 441–42, 446, 449–50, 455, 344, 346, 348, 360, 364, 367, 369, 393, Abell, George Ogden (1927–1983), 47, 475, 516 395, 395, 396–404, 406, 410, 415, 248 Austin, Edward P. (1843–1906), 6, 82, 423–24, 436, 441, 446, 448, 450, 455, Abbott, Francis Preserved (1799–1883), 335, 337, 446, 450 458–59, 461–63, 470, 477, 481, 483, 517–19 Auwers, Georg Friedrich Julius Arthur v. 505–11, 513–14, 517, 520, 526, 533, Abney, William (1843–1920), 360 (1838–1915), 7, 10, 12, 14–15, 26–27, 540–42, 548–61 Adams, John Couch (1819–1892), 122, 47, 50–51, 61, 65, 68–69, 88, 92–93, -
Rings in the Haloes of Planetary Nebulae
A&A 417, 637–646 (2004) Astronomy DOI: 10.1051/0004-6361:20034420 & c ESO 2004 Astrophysics Rings in the haloes of planetary nebulae R. L. M. Corradi1,P.S´anchez-Bl´azquez2 ,G.Mellema3,,C.Gianmanco4, and H. E. Schwarz5 1 Isaac Newton Group of Telescopes, Ap. de Correos 321, 38700 Sta. Cruz de la Palma, Spain 2 Departamento de Astrof´ısica, Universidad Complutense, 28040, Madrid, Spain e-mail: [email protected] 3 Sterrewacht Leiden, Postbus 9513, 2300 RA Leiden, The Netherlands e-mail: [email protected] 4 Instituto de Astrof´ısica de Canarias, 38200 La Laguna, Tenerife, Spain e-mail: [email protected] 5 Cerro Tololo Inter-American Observatory, NOAO-AURA, Casilla 603, La Serena, Chile e-mail: [email protected] Received 30 September 2003 / Accepted 17 December 2003 Abstract. We present a search for rings or arcs in the haloes of planetary nebulae (PNe). We discovered such structures in eight PNe, tripling the sample of PNe with known rings. This shows that, contrary to what was believed to date, the occurrence of mass loss fluctuations with timescales of 102–103 yrs at the end of the asymptotic giant branch phase (AGB) is common. We estimate a lower limit of the occurrence rate of rings in PN haloes to be ∼35%. Using these new detections and the cases previously known, we discuss the statistical properties of ring systems in PNe haloes. We estimate that the mass modulation producing the rings takes place during the last 10 000 or 20 000 yrs of AGB evolution. -
Zur Objektauswahl: Nummer Anklicken Sternbild- Übersicht NGC
NGC-Objektauswahl Cygnus NGC 6764 NGC 6856 NGC 6910 NGC 6995 NGC 7031 NGC 7082 NGC 6798 NGC 6857 NGC 6913 NGC 7037 NGC 7086 NGC 6801 NGC 6866 NGC 6914 NGC 6996 NGC 7039 NGC 7092 NGC 6811 NGC 6871 NGC 6916 NGC 6997 NGC 7044 NGC 7093 NGC 6819 NGC 6874 NGC 6946 NGC 7000 NGC 7048 NGC 7116 NGC 6824 NGC 6881 NGC 6960 NGC 7008 NGC 7050 NGC 7127 NGC 6826 NGC 6883 NGC 6974 NGC 7013 NGC 7058 NGC 7128 NGC 6833 NGC 6884 NGC 6979 NGC 7024 NGC 7062 NGC 6834 NGC 6888 NGC 6991 NGC 7026 NGC 7063 NGC 6846 NGC 6894 NGC 6992 NGC 7027 NGC 7067 Sternbild- Übersicht Zur Objektauswahl: Nummer anklicken Sternbildübersicht Auswahl NGC 6764 Aufsuchkarte Auswahl NGC 6798 _6801_6824_Aufsuchkarte Auswahl NGC 6811 Aufsuchkarte Auswahl NGC 6819 Aufsuchkarte Auswahl NGC 6826 Aufsuchkarte Auswahl NGC 6833 Aufsuchkarte Auswahl NGC 6834 Aufsuchkarte Auswahl NGC 6846_6857 Aufsuchkarte Auswahl NGC 6856 Aufsuchkarte Auswahl NGC 6866_6884 Aufsuchkarte Auswahl NGC 6871_6883 Aufsuchkarte Auswahl NGC 6874_6881_6888_6913 Aufsuchkarte Auswahl NGC 6894 Aufsuchkarte Auswahl NGC 6910_6914 Aufsuchkarte Auswahl NGC 6916_6946 Aufsuchkarte Auswahl NGC 6960_6974_6979_6992_6995_7013 Aufsuchkarte Auswahl NGC6991_96_97_7000_26_39_48 Aufsuchkarte Auswahl NGC 7008_7031_7058_7086_7127_7128 Aufsuchkarte Auswahl NGC 7024_7027_7044 Aufsuchkarte Auswahl N 7037_7050_7063 Aufsuchkarte Auswahl NGC 7062_7067_7082_7092_7093 Aufsuchkarte Auswahl NGC 7116 Aufsuchkarte Auswahl NGC 6764_Übersichtskarte Aufsuch- Auswahl karte NGC 6798 Übersichtskarte Aufsuch- Auswahl karte NGC 6801 Übersichtskarte Aufsuch- -
IAUS283 Planetary Nebulae: an Eye to the Future P R O G R a M M E & a B S T R a C
IAUS283 Planetary Nebulae: An Eye to the Future P A R B O S G T R & R A A M C M T E S 25-29 July, 2011 Puerto de La Cruz Conference Centre Tenerife, Canary Islands, Spain Organized by INSTITUTO DE ASTROFÍSICA DE CANARIAS IAUS283: Planetary Nebulae. An Eye to the Future SPONSORS The Local Organizing Committee is greatly indebted to the following entities that provided financial support in different ways: INTERNATIONAL ASTRONOMICAL UNION (IAU) MINISTERIO DE CIENCIA E INNOVACIÓN (MICINN) INSTITUTO DE ASTROFÍSICA DE CANARIAS (IAC) 1 IAUS283: Planetary Nebulae. An Eye to the Future TABLE OF CONTENTS Invited Speakers, SOC & LOC 3 Social Programme Information 4 Scientific Programme 5 Invited Reviews and Contributed Talks 8 Session 1: New Results from Observations 9 Session 2: The Stellar Evolution Connection 23 2a: Through the AGB and Beyond 24 2b: Aspects of the PN Phase 33 2c: Aspects of the Central Stars 47 Session 3: The Cosmic Population of Galactic and Extragalactic PNe 58 Session 4: Future Endeavours in the Field 71 Posters 74 List of Participants 121 Useful Information 124 Notes 128 2 IAUS283: Planetary Nebulae. An Eye to the Future INVITED SPEAKERS, SOC & LOC Invited Speakers (IS) ♦ M. Arnaboldi (ESO) ♦ X.-W. Liu (China) ♦ B. Balick (USA) ♦ V. Luridiana (Spain) ♦ M. Barlow (UK) ♦ L. Magrini (Italy) ♦ L. Bianchi (USA) ♦ P. Marigo (Italy) ♦ Y.-H. Chu (USA) ♦ Q. Parker (Australia) ♦ A. García-Hernandez (Spain) ♦ W. Reid (Australia) ♦ P. García-Lario (ESA) ♦ M. Richer (Mexico) ♦ M. Guerrero (Spain) ♦ R. Shaw (USA) ♦ R. Izzard (Germany) ♦ W. Steffen (Mexico) ♦ H.