Navigating North America
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Our Place in the Universe (239 Pages)
OUR PLACE IN THE uNIVERSE Norman k. Glendenning Lawrence Berkeley National Laboratiry World scientific Imperial College Press Published by Imperial College Press 57 Shelton Street Covent Garden London WC2H 9HE and World Scientific Publishing Co. Pte. Ltd. 5 Toh Tuck Link, Singapore 596224 USA office: 27 Warren Street, Suite 401-402, Hackensack, NJ 07601 UK office: 57 Shelton Street, Covent Garden, London WC2H 9HE Library of Congress Cataloging-in-Publication Data Glendenning, Norman K. Our place in the universe / Norman K. Glendenning. p. cm. Includes bibliographical references and index. ISBN-13 978-981-270-068-1 -- ISBN-10 981-270-068-4 ISBN-13 978-981-270-069-8 (pbk) -- ISBN-10 981-270-069-2 (pbk) 1. Cosmology. 2. Galaxies--Formation. 3. Galaxies--Evolution. 4. Astrophysics. 5. Solar system--Origin. I. Title. QB981 .G585 2007 523.1--dc22 British Library Cataloguing-in-Publication Data A catalogue record for this book is available from the British Library. Cover picture: The Horsehead is a reflection nebula; it is located in the much larger Orion Nebula, an immense molecular cloud of primordial hydrogen and helium, together dust cast off by the surfaces of stars. The clouds that form the Horsehead are illuminated from behind by a stellar nursery of young bright stars. Credit: Photo taken at Mauna Kea, Hawaii with the Canada-France-Hawaii Telescope. Copyright © 2007 by Imperial College Press and World Scientific Publishing Co. Pte. Ltd. All rights reserved. This book, or parts thereof, may not be reproduced in any form or by any means, electronic or mechanical, including photocopying, recording or any information storage and retrieval system now known or to be invented, without written permission from the Publisher. -
BRAS Newsletter August 2013
www.brastro.org August 2013 Next meeting Aug 12th 7:00PM at the HRPO Dark Site Observing Dates: Primary on Aug. 3rd, Secondary on Aug. 10th Photo credit: Saturn taken on 20” OGS + Orion Starshoot - Ben Toman 1 What's in this issue: PRESIDENT'S MESSAGE....................................................................................................................3 NOTES FROM THE VICE PRESIDENT ............................................................................................4 MESSAGE FROM THE HRPO …....................................................................................................5 MONTHLY OBSERVING NOTES ....................................................................................................6 OUTREACH CHAIRPERSON’S NOTES .........................................................................................13 MEMBERSHIP APPLICATION .......................................................................................................14 2 PRESIDENT'S MESSAGE Hi Everyone, I hope you’ve been having a great Summer so far and had luck beating the heat as much as possible. The weather sure hasn’t been cooperative for observing, though! First I have a pretty cool announcement. Thanks to the efforts of club member Walt Cooney, there are 5 newly named asteroids in the sky. (53256) Sinitiere - Named for former BRAS Treasurer Bob Sinitiere (74439) Brenden - Named for founding member Craig Brenden (85878) Guzik - Named for LSU professor T. Greg Guzik (101722) Pursell - Named for founding member Wally Pursell -
A Campus Observatory Image of the North America Nebula
The Observer A Campus Observatory Image of the North America Nebula by Fred Ringwald Fresno State’s Campus Observatory is convenient for students to use, but its sky rates 10 on the Bortle scale: “Most people don’t look up.” The faintest stars the unaided eye can see there are about 3rd magnitude. Nevertheless, its telescopes can get good images through an Hα (pronounced “H-alpha”) filter. An Hα filter passes only a narrow band of wavelengths that are centered on the Hα line, the scarlet wavelength at which hydrogen radiates the most light visible to the eye. City lights radiate mostly at other wavelengths, from mercury or sodium vapor in the lamps. Hydrogen is the most common element in nebulae, so Hα filters improve their image contrast. This image was taken through a 70-mm guidescope mounted piggyback on the Campus Observatory’s main telescope. The guidescope was made by Vixen. With a focal length of only 400 mm, the guidescope gets a wide field of view, which makes it easier for novice students to point the telescope. With the SBIG ST-9 camera used to take this image, the field of view is 1.5º on a side. It shows the southern end of NGC 7000, called “the North America Nebula” because of its shape. At upper right is “Florida,” bounded by a dust lane corresponding to the “Gulf of Mexico”; at bottom-center is “Mexico.” A bright shock front runs through the east side (on the left), which is called “the Great Wall,” incongruous since that’s in China! The North America Nebula is in the constellation Cygnus, 3º east of the 1st-magntude supergiant star Deneb. -
Star Formation in the “Gulf of Mexico”
A&A 528, A125 (2011) Astronomy DOI: 10.1051/0004-6361/200912671 & c ESO 2011 Astrophysics Star formation in the “Gulf of Mexico” T. Armond1,, B. Reipurth2,J.Bally3, and C. Aspin2, 1 SOAR Telescope, Casilla 603, La Serena, Chile e-mail: [email protected] 2 Institute for Astronomy, University of Hawaii at Manoa, 640 N. Aohoku Place, Hilo, HI 96720, USA e-mail: [reipurth;caa]@ifa.hawaii.edu 3 Center for Astrophysics and Space Astronomy, University of Colorado, Boulder, CO 80309, USA e-mail: [email protected] Received 9 June 2009 / Accepted 6 February 2011 ABSTRACT We present an optical/infrared study of the dense molecular cloud, L935, dubbed “The Gulf of Mexico”, which separates the North America and the Pelican nebulae, and we demonstrate that this area is a very active star forming region. A wide-field imaging study with interference filters has revealed 35 new Herbig-Haro objects in the Gulf of Mexico. A grism survey has identified 41 Hα emission- line stars, 30 of them new. A small cluster of partly embedded pre-main sequence stars is located around the known LkHα 185-189 group of stars, which includes the recently erupting FUor HBC 722. Key words. Herbig-Haro objects – stars: formation 1. Introduction In a grism survey of the W80 region, Herbig (1958) detected a population of Hα emission-line stars, LkHα 131–195, mostly The North America nebula (NGC 7000) and the adjacent Pelican T Tauri stars, including the little group LkHα 185 to 189 located nebula (IC 5070), both well known for the characteristic shapes within the dark lane of the Gulf of Mexico, thus demonstrating that have given rise to their names, are part of the single large that low-mass star formation has recently taken place here. -
Binocular Challenge Here
AHSP Binocular Observing Award Compiled by Phil Harrington www.philharrington.net • To qualify for the BOA pin, you must see 15 of the following 20 binocular targets. Check off each as you spot them. Seen # Object Const. Type* RA Dec Mag Size Nickname 1. M13 Her GC 16 41.7 +36 28 5.9 16' Great Hercules Globular 2. M57 Lyr PN 18 53.6 +33 02 9.7 86"x62" Ring Nebula 3. Collinder 399 Vul AS 19 25.4 +20 11 3.6 60' Coathanger/Brocchi’s Cluster 3.1 4. Albireo Cyg Dbl 19 30.7 +27 57 35” Color Contrasting Double 5.1 5. M27 Vul PN 19 59.6 +22 43 8.1 8’x6’ Dumbbell Nebula 6. NGC 6992 Cyg SNR 20 56.4 +31 43 - 60'x8 Veil Nebula (east) 7. NGC 7000 Cyg BN 20 58.8 +44 20 - 120'x100' North America Nebula 8. M15 Peg GC 21 30.0 +12 10 7.5 12’ Great Pegasus Cluster 9. M39 Cyg OC 21 32.2 +48 26 4.6 32' 10. Barnard 168 Cyg DN 21 53.2 +47 12 - 100'x10' West of Cocoon Nebula 11. IC 5146 Cyg BN/OC 21 53.5 +47 16 - 12'x12' Cocoon Nebula 12. M110 And Gx 00 40.4 +41 41 10 17’x10’ 13. M32 And Gx 00 42.8 +40 52 10 8’x6’ 14. M31 And Gx 00 42.8 +41 16 4.5 178’ Andromeda Galaxy 15. NGC 457 Cas OC 01 19.1 +58 20 6.4 13’ Owl Cluster/ET Cluster 16. -
A Basic Requirement for Studying the Heavens Is Determining Where In
Abasic requirement for studying the heavens is determining where in the sky things are. To specify sky positions, astronomers have developed several coordinate systems. Each uses a coordinate grid projected on to the celestial sphere, in analogy to the geographic coordinate 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 is probably the most widely used celestial coordinate system. It is also the one most closely related to the geographic coordinate system, because they use the same fun damental plane and the same poles. The projection of the Earth's equator onto the celestial sphere is called the celestial equator. Similarly, projecting the geographic poles on to the celest ial sphere defines the north and south celestial poles. However, there is an important difference between the equatorial and geographic coordinate systems: the geographic system is fixed to the Earth; it 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 of course 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. The longitud inal angle is called the right ascension (RA for short). -
LIST of PUBLICATIONS Aryabhatta Research Institute of Observational Sciences ARIES (An Autonomous Scientific Research Institute
LIST OF PUBLICATIONS Aryabhatta Research Institute of Observational Sciences ARIES (An Autonomous Scientific Research Institute of Department of Science and Technology, Govt. of India) Manora Peak, Naini Tal - 263 129, India (1955−2020) ABBREVIATIONS AA: Astronomy and Astrophysics AASS: Astronomy and Astrophysics Supplement Series ACTA: Acta Astronomica AJ: Astronomical Journal ANG: Annals de Geophysique Ap. J.: Astrophysical Journal ASP: Astronomical Society of Pacific ASR: Advances in Space Research ASS: Astrophysics and Space Science AE: Atmospheric Environment ASL: Atmospheric Science Letters BA: Baltic Astronomy BAC: Bulletin Astronomical Institute of Czechoslovakia BASI: Bulletin of the Astronomical Society of India BIVS: Bulletin of the Indian Vacuum Society BNIS: Bulletin of National Institute of Sciences CJAA: Chinese Journal of Astronomy and Astrophysics CS: Current Science EPS: Earth Planets Space GRL : Geophysical Research Letters IAU: International Astronomical Union IBVS: Information Bulletin on Variable Stars IJHS: Indian Journal of History of Science IJPAP: Indian Journal of Pure and Applied Physics IJRSP: Indian Journal of Radio and Space Physics INSA: Indian National Science Academy JAA: Journal of Astrophysics and Astronomy JAMC: Journal of Applied Meterology and Climatology JATP: Journal of Atmospheric and Terrestrial Physics JBAA: Journal of British Astronomical Association JCAP: Journal of Cosmology and Astroparticle Physics JESS : Jr. of Earth System Science JGR : Journal of Geophysical Research JIGR: Journal of Indian -
Sky & Telescope
Eclipse from the See Sirius B: The Nearest Spot the Other EDGE OF SPACE p. 66 WHITE DWARF p. 30 BLUE PLANETS p. 50 THE ESSENTIAL GUIDE TO ASTRONOMY What Put the Bang in the Big Bang p. 22 Telescope Alignment Made Easy p. 64 Explore the Nearby Milky Way p. 32 How to Draw the Moon p. 54 OCTOBER 2013 Cosmic Gold Rush Racing to fi nd exploding stars p. 16 Visit SkyandTelescope.com Download Our Free SkyWeek App FC Oct2013_J.indd 1 8/2/13 2:47 PM “I can’t say when I’ve ever enjoyed owning anything more than my Tele Vue products.” — R.C, TX Tele Vue-76 Why Are Tele Vue Products So Good? Because We Aim to Please! For over 30-years we’ve created eyepieces and telescopes focusing on a singular target; deliver a cus- tomer experience “...even better than you imagined.” Eyepieces with wider, sharper fields of view so you see more at any power, Rich-field refractors with APO performance so you can enjoy Andromeda as well as Jupiter in all their splendor. Tele Vue products complement each other to pro- vide an observing experience as exquisite in performance as it is enjoyable and effortless. And how do we score with our valued customers? Judging by superlatives like: “in- credible, truly amazing, awesome, fantastic, beautiful, work of art, exceeded expectations by a mile, best quality available, WOW, outstanding, uncom- NP101 f/5.4 APO refractor promised, perfect, gorgeous” etc., BULLSEYE! See these superlatives in with 110° Ethos-SX eye- piece shown on their original warranty card context at TeleVue.com/comments. -
October 2020
The Newsletter of Westchester Amateur Astronomers October 2020 Pelican Nebula (IC 5070 and 5067) by Olivier Prache Imaged from Olivier’s observatory in Pleasantville. Borg 101ED and ZWO ASI071MC one-shot-color camera using an Optolong L-Enhance filter. Three hours of five-minute subs (unguided) and a bit of work with PixInsight. SERVING THE ASTRONOMY COMMUNITY SINCE 1986 1 Westchester Amateur Astronomers SkyWAAtch October 2020 WAA October Meeting WAA November Meeting Friday, October 2 at 7:30 pm Friday, November at 6 7:30 pm On-line via Zoom On-line via Zoom Intelligent Nighttime Lighting: The Many BLACK HOLES: Not so black? Benefits of Dark Skies Willie Yee Charles Fulco Recent years have seen major breakthroughs in the Science educator Charles Fulco will discuss the meth- study of black holes, including the first image of a ods and many benefits of reducing light pollution, black hole from the Event Horizon Telescope and the including energy and tax dollar savings, health bene- detection of black hole collisions with the Laser fits and of course seeing the Milky Way again. Invita- Interferometer Gravitational-wave Observatory. tions and log-in instructions will be sent to WAA Dr. Yee, a NASA Solar System Ambassador and Past members via email. President of the Mid-Hudson Astronomical Association, will review the basic science of black Starway to Heaven holes and the myths surrounding them, and present Ward Pound Ridge Reservation, the recent findings of these projects. Cross River, NY Call: 1-877-456-5778 (toll free) for announcements, Scheduled for Oct 10th (rain/cloud date Oct 17). -
A Compendium of Distances to Molecular Clouds in the Star Formation Handbook?,?? Catherine Zucker1, Joshua S
A&A 633, A51 (2020) Astronomy https://doi.org/10.1051/0004-6361/201936145 & c ESO 2020 Astrophysics A compendium of distances to molecular clouds in the Star Formation Handbook?,?? Catherine Zucker1, Joshua S. Speagle1, Edward F. Schlafly2, Gregory M. Green3, Douglas P. Finkbeiner1, Alyssa Goodman1,5, and João Alves4,5 1 Center for Astrophysics | Harvard & Smithsonian, 60 Garden St., Cambridge, MA 02138, USA e-mail: [email protected], [email protected] 2 Lawrence Berkeley National Laboratory, One Cyclotron Road, Berkeley, CA 94720, USA 3 Kavli Institute for Particle Astrophysics and Cosmology, Physics and Astrophysics Building, 452 Lomita Mall, Stanford, CA 94305, USA 4 University of Vienna, Department of Astrophysics, Türkenschanzstraße 17, 1180 Vienna, Austria 5 Radcliffe Institute for Advanced Study, Harvard University, 10 Garden St, Cambridge, MA 02138, USA Received 21 June 2019 / Accepted 12 August 2019 ABSTRACT Accurate distances to local molecular clouds are critical for understanding the star and planet formation process, yet distance mea- surements are often obtained inhomogeneously on a cloud-by-cloud basis. We have recently developed a method that combines stellar photometric data with Gaia DR2 parallax measurements in a Bayesian framework to infer the distances of nearby dust clouds to a typical accuracy of ∼5%. After refining the technique to target lower latitudes and incorporating deep optical data from DECam in the southern Galactic plane, we have derived a catalog of distances to molecular clouds in Reipurth (2008, Star Formation Handbook, Vols. I and II) which contains a large fraction of the molecular material in the solar neighborhood. Comparison with distances derived from maser parallax measurements towards the same clouds shows our method produces consistent distances with .10% scatter for clouds across our entire distance spectrum (150 pc−2.5 kpc). -
Binocular Observing Olympics Stellafane 2018
Binocular Observing Olympics Stellafane 2018 Compiled by Phil Harrington www.philharrington.net • To qualify for the BOO pin, you must see 15 of the following 20 binocular targets. Check off each as you spot them. Seen # Object Const. Type* RA Dec Mag Size Nickname 1. M4 Sco GC 16 23.6 -26 32 6.0 26' Cat’s Eye Globular 2. M13 Her GC 16 41.7 +36 28 5.9 16' Great Hercules Globular 3. M6 Sco OC 17 40.1 -32 13 4.2 15' Butterfly Cluster 4. IC 4665 Oph OC 17 46.3 +05 43 4.2 41' Summer Beehive 5. M7 Sco OC 17 53.9 -34 49 3.3 80' Ptolemy’s Cluster 6. M20 Sgr BN/OC 18 02.6 -23 02 8.5 29'x27' Trifid Nebula 7. M8 Sgr BN/OC 18 03.8 -24 23 5.8 90'x40' Lagoon Nebula 8. M17 Sgr BN 18 20.8 -16 11 7 46'x37' Swan or Omega Nebula 9. M22 Sgr GC 18 36.4 -23 54 5.1 24' Great Sagittarius Cluster 10. M11 Sct OC 18 51.1 -06 16 5.8 14' Wild Duck Cluster 11. M57 Lyr PN 18 53.6 +33 02 9.7 70"x150" Ring Nebula 12. Collinder 399 Vul AS 19 25.4 +20 11 3.6 60' Coathanger/Brocchi’s Cluster 13. PK 64+5.1 Cyg PN 19 34.8 +30 31 9.6p 8" Campbell's Hydrogen Star 14. M27 Vul PN 19 59.6 +22 43 8.1 8’x6’ Dumbbell Nebula 15. -
Quiz 1 Spring 1995
Phys 102 Astronomy Name _____________________Key STELLAR EVOLUTION IN THE SKY 57 1) On the diagram below, neatly (TAKE TIME TO BE NEAT AND CAREFUL IN YOUR WORK!) a)10 Sketch the constellation lines & label Lyra, Cygnus, Aquila, The Keystone and The Teapot. b)32 Using DIFFERENT COLORS for different LUMINOSITY classes, label the stars Vega, Sheliak, Sulaphat,Alberio, Sadr, Altair, Tarazed, Denebokab (δ Aql), Althalimain (λ Aql), Dabih (β Cap), Deneb Algeidi (δ Cap), ζ Her, Ras Algethi (α Her), Kornephoros (β Her), Antares (α Sco), and Kaus Borealis (λ Sgr), with their name and spectral type. (Use the colors indicated in the legend! Deneb is shown as an example) c)15 Indicate the positions of Lagoon, Eagle, Ring, and Veil Nebulas and Cyg. X-1, and state the type of object and the stage of stellar evolution taking place in each (the North America Nebula is an example). GALACTIC EQUATOR I North America Nebula II Deneb A2 I Emission Nebula III Star birth ZENITH IV CYGNUS The Sadr F8 I Keystone V LYRA Vega A0 V ζ Her G1 IV Sulaphat Sheliak B7 V B9 II Alberio Ring Nebula in Lyra Cyg X-1 Black Hole K3 II + B9.5 V Planetary Nebula: Star Death Kornephoros Star death G7 III Veil Nebula in Cygnus Supernova Remnant: Star death Ras Algethi M5 I-II Tarazed K3 II AQUILA Altair A7 V Denebokab F2 IV C ELESTIAL EQUATOR Althalimain B9 V Deneb Algeidi A3 IV Eagle Nebula in Scutum OPHIUCHUS Emission Nebula Dabih Star formation K0 II + A5 V Kaus Borealis ATURN JUPITER CAPRICORNUS S K1 III ECLIPTIC Lagoon Nebula in Sagittarius Emission Nebula GALACTIC Star formation Antares M1.5 I Starry Night view from CENTER Canton, New York, SAGITTARIUS 6:00 pm, October 21, 2019 .