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Messier Objects
Messier Objects From the Stocker Astroscience Center at Florida International University Miami Florida The Messier Project Main contributors: • Daniel Puentes • Steven Revesz • Bobby Martinez Charles Messier • Gabriel Salazar • Riya Gandhi • Dr. James Webb – Director, Stocker Astroscience center • All images reduced and combined using MIRA image processing software. (Mirametrics) What are Messier Objects? • Messier objects are a list of astronomical sources compiled by Charles Messier, an 18th and early 19th century astronomer. He created a list of distracting objects to avoid while comet hunting. This list now contains over 110 objects, many of which are the most famous astronomical bodies known. The list contains planetary nebula, star clusters, and other galaxies. - Bobby Martinez The Telescope The telescope used to take these images is an Astronomical Consultants and Equipment (ACE) 24- inch (0.61-meter) Ritchey-Chretien reflecting telescope. It has a focal ratio of F6.2 and is supported on a structure independent of the building that houses it. It is equipped with a Finger Lakes 1kx1k CCD camera cooled to -30o C at the Cassegrain focus. It is equipped with dual filter wheels, the first containing UBVRI scientific filters and the second RGBL color filters. Messier 1 Found 6,500 light years away in the constellation of Taurus, the Crab Nebula (known as M1) is a supernova remnant. The original supernova that formed the crab nebula was observed by Chinese, Japanese and Arab astronomers in 1054 AD as an incredibly bright “Guest star” which was visible for over twenty-two months. The supernova that produced the Crab Nebula is thought to have been an evolved star roughly ten times more massive than the Sun. -
Globular Clusters and Galactic Nuclei
Scuola di Dottorato “Vito Volterra” Dottorato di Ricerca in Astronomia– XXIV ciclo Globular Clusters and Galactic Nuclei Thesis submitted to obtain the degree of Doctor of Philosophy (“Dottore di Ricerca”) in Astronomy by Alessandra Mastrobuono Battisti Program Coordinator Thesis Advisor Prof. Roberto Capuzzo Dolcetta Prof. Roberto Capuzzo Dolcetta Anno Accademico 2010-2011 ii Abstract Dynamical evolution plays a key role in shaping the current properties of star clus- ters and star cluster systems. We present the study of stellar dynamics both from a theoretical and numerical point of view. In particular we investigate this topic on different astrophysical scales, from the study of the orbital evolution and the mutual interaction of GCs in the Galactic central region to the evolution of GCs in the larger scale galactic potential. Globular Clusters (GCs), very old and massive star clusters, are ideal objects to explore many aspects of stellar dynamics and to investigate the dynamical and evolutionary mechanisms of their host galaxy. Almost every surveyed galaxy of sufficiently large mass has an associated group of GCs, i.e. a Globular Cluster System (GCS). The first part of this Thesis is devoted to the study of the evolution of GCSs in elliptical galaxies. Basing on the hypothesis that the GCS and stellar halo in a galaxy were born at the same time and, so, with the same density distribution, a logical consequence is that the presently observed difference may be due to evolution of the GCS. Actually, in this scenario, GCSs evolve due to various mechanisms, among which dynamical friction and tidal interaction with the galactic field are the most important. -
The Messier Catalog
The Messier Catalog Messier 1 Messier 2 Messier 3 Messier 4 Messier 5 Crab Nebula globular cluster globular cluster globular cluster globular cluster Messier 6 Messier 7 Messier 8 Messier 9 Messier 10 open cluster open cluster Lagoon Nebula globular cluster globular cluster Butterfly Cluster Ptolemy's Cluster Messier 11 Messier 12 Messier 13 Messier 14 Messier 15 Wild Duck Cluster globular cluster Hercules glob luster globular cluster globular cluster Messier 16 Messier 17 Messier 18 Messier 19 Messier 20 Eagle Nebula The Omega, Swan, open cluster globular cluster Trifid Nebula or Horseshoe Nebula Messier 21 Messier 22 Messier 23 Messier 24 Messier 25 open cluster globular cluster open cluster Milky Way Patch open cluster Messier 26 Messier 27 Messier 28 Messier 29 Messier 30 open cluster Dumbbell Nebula globular cluster open cluster globular cluster Messier 31 Messier 32 Messier 33 Messier 34 Messier 35 Andromeda dwarf Andromeda Galaxy Triangulum Galaxy open cluster open cluster elliptical galaxy Messier 36 Messier 37 Messier 38 Messier 39 Messier 40 open cluster open cluster open cluster open cluster double star Winecke 4 Messier 41 Messier 42/43 Messier 44 Messier 45 Messier 46 open cluster Orion Nebula Praesepe Pleiades open cluster Beehive Cluster Suburu Messier 47 Messier 48 Messier 49 Messier 50 Messier 51 open cluster open cluster elliptical galaxy open cluster Whirlpool Galaxy Messier 52 Messier 53 Messier 54 Messier 55 Messier 56 open cluster globular cluster globular cluster globular cluster globular cluster Messier 57 Messier -
Introduction to Astronomical Photometry, Second Edition
This page intentionally left blank Introduction to Astronomical Photometry, Second Edition Completely updated, this Second Edition gives a broad review of astronomical photometry to provide an understanding of astrophysics from a data-based perspective. It explains the underlying principles of the instruments used, and the applications and inferences derived from measurements. Each chapter has been fully revised to account for the latest developments, including the use of CCDs. Highly illustrated, this book provides an overview and historical background of the subject before reviewing the main themes within astronomical photometry. The central chapters focus on the practical design of the instruments and methodology used. The book concludes by discussing specialized topics in stellar astronomy, concentrating on the information that can be derived from the analysis of the light curves of variable stars and close binary systems. This new edition includes numerous bibliographic notes and a glossary of terms. It is ideal for graduate students, academic researchers and advanced amateurs interested in practical and observational astronomy. Edwin Budding is a research fellow at the Carter Observatory, New Zealand, and a visiting professor at the Çanakkale University, Turkey. Osman Demircan is Director of the Ulupınar Observatory of Çanakkale University, Turkey. Cambridge Observing Handbooks for Research Astronomers Today’s professional astronomers must be able to adapt to use telescopes and interpret data at all wavelengths. This series is designed to provide them with a collection of concise, self-contained handbooks, which covers the basic principles peculiar to observing in a particular spectral region, or to using a special technique or type of instrument. The books can be used as an introduction to the subject and as a handy reference for use at the telescope, or in the office. -
Deep Sky Explorer Atlas
Deep Sky Explorer Atlas Reference manual Star charts for the southern skies Compiled by Auke Slotegraaf and distributed under an Attribution-Noncommercial 3.0 Creative Commons license. Version 0.20, January 2009 Deep Sky Explorer Atlas Introduction Deep Sky Explorer Atlas Reference manual The Deep Sky Explorer’s Atlas consists of 30 wide-field star charts, from the south pole to declination +45°, showing all stars down to 8th magnitude and over 1 000 deep sky objects. The design philosophy of the Atlas was to depict the night sky as it is seen, without the clutter of constellation boundary lines, RA/Dec fiducial markings, or other labels. However, constellations are identified by their standard three-letter abbreviations as a minimal aid to orientation. Those wishing to use charts showing an array of invisible lines, numbers and letters will find elsewhere a wide selection of star charts; these include the Herald-Bobroff Astroatlas, the Cambridge Star Atlas, Uranometria 2000.0, and the Millenium Star Atlas. The Deep Sky Explorer Atlas is very much for the explorer. Special mention should be made of the excellent charts by Toshimi Taki and Andrew L. Johnson. Both are free to download and make ideal complements to this Atlas. Andrew Johnson’s wide-field charts include constellation figures and stellar designations and are highly recommended for learning the constellations. They can be downloaded from http://www.cloudynights.com/item.php?item_id=1052 Toshimi Taki has produced the excellent “Taki’s 8.5 Magnitude Star Atlas” which is a serious competitor for the commercial Uranometria atlas. His atlas has 149 charts and is available from http://www.asahi-net.or.jp/~zs3t-tk/atlas_85/atlas_85.htm Suggestions on how to use the Atlas Because the Atlas is distributed in digital format, its pages can be printed on a standard laser printer as needed. -
ASSA Top 100 Deep Sky Objects
# Object ID Bennett ID Type Size Con RA Dec D Vis Interesting Facts Distance from Discoverer Earth (light- years) 1 NGC 55, LEDA 1014 Glxy 32’x5.6’ Scl 00 15 – 39 11 06,25 Sep–Feb The String of Pearls. A barred galaxy that is 7200000 James Dunlop on August 4, 1826 edge-on to us. It has a bright elongated center with a small round cloud to the east of it. If you look to the side of it while still concentrating on the object you might be able to see additional bright clouds and dark Ben 1 rifts in this galaxy. 2 NGC 104, 47 Tucanae Glcl 31’ Tuc 00 24 – 72 05 05,06 Sep–Feb The cluster appears roughly the size of the 16700 Abbe Lacaille from South Africa, 1751. At the full moon in the sky under ideal conditions. Cape, Abbé wanted to test Newton's theory of It is the second brightest globular cluster in gravitation and verify the shape of the earth in the the sky (after Omega Centauri), and is southern hemisphere. His results suggested the noted for having a very bright and dense Earth was egg-shaped not oval. In 1838, Thomas core. It is also one of the most massive Maclear who was Astronomer Royal at the Cape, globular clusters in the Milky Way, repeated the measurements. He found that de containing millions of stars Lacaille had failed to take into account the gravitational attraction of the nearby mountains. Ben 2 3 NGC 247, LEDA 2758 Glxy 18’ x 5’ Cet 00 47 – 20 46 06,25 Sep–Feb Very dusty galaxy therefore not bright, 11000000 ? Ben 3 magnitude 9.2, challenging to find. -
Multiple Galaxies - F
Multiple Galaxies - F. Zwicky file:///e|/moe/HTML/March02/Zwicky/Zwicky.htm MULTIPLE GALAXIES F. Zwicky Table of Contents DEFINITIONS REMARKS ON THE HISTORY OF THE SUBJECT A. Small Groups of Galaxies Clusters of Galaxies Recent Advances Instrumentation WIDELY SEPARATED INTERCONNECTED GALAXIES The Triple System IC 3481, Anon, IC 3483 KEENAN's System Another Remarkable Filamentary Structure WILD'S Triple Galaxy The Basic Types of Structures Some Conclusions LONG EXTENSIONS AND SPURS OF SINGLE AND OF MULTIPLE GALAXIES NGC 4038-4039 NGC 750-751 A System in Leo NGC 4651 and Dwarf Companion NGC 3628 and Faint Extensions Spiral Galaxy with One Long Arm SOME SPECIAL PROBLEMS The Milky Way System and the Magellanic Clouds The Andromeda Nebula and its Companions New Clues on the Sense of Rotation of Spiral Galaxies Multiple Galaxies in Clusters and in the General Field OUTLOOK AND PROGRAMS REFERENCES 1. DEFINITIONS The meaning of the term multiple galaxies obviously can be clear only if we know what an individual galaxy is. Unfortunately it is not at the present time possible to give an exact definition of a galaxy as a physical stellar system which is in practice operationally useful. Theoretically one might postulate that any agglomeration of stars, gases and solid particles constitutes a galaxy if its various material components cannot escape directly from this agglomeration. A stellar system or galaxy is therefore a cohesive unit of stars, dust and gases within which only a fraction of its components possess velocities high enough to allow them to escape and to make their way to the vast intergalactic spaces. -
Charles Messier (1730-1817) Was an Observational Astronomer Working
Charles Messier (1730-1817) was an observational Catalogue (NGC) which was being compiled at the same astronomer working from Paris in the eighteenth century. time as Messier's observations but using much larger tele He discovered between 15 and 21 comets and observed scopes, probably explains its modern popularity. It is a many more. During his observations he encountered neb challenging but achievable task for most amateur astron ulous objects that were not comets. Some of these objects omers to observe all the Messier objects. At «star parties" were his own discoveries, while others had been known and within astronomy clubs, going for the maximum before. In 1774 he published a list of 45 of these nebulous number of Messier objects observed is a popular competi objects. His purpose in publishing the list was so that tion. Indeed at some times of the year it is just about poss other comet-hunters should not confuse the nebulae with ible to observe most of them in a single night. comets. Over the following decades he published supple Messier observed from Paris and therefore the most ments which increased the number of objects in his cata southerly object in his list is M7 in Scorpius with a decli logue to 103 though objects M101 and M102 were in fact nation of -35°. He also missed several objects from his list the same. Later other astronomers added a replacement such as h and X Per and the Hyades which most observers for M102 and objects 104 to 110. It is now thought proba would feel should have been included. -
October 2017
Page 1 Monthly Newsletter of the Durban Centre - October 2017 Page 2 Table of Contents Chairman’s Chatter …...……………………………………...….…… 3 A Stroll Through The Stars Of Capricorn ……………………….... 5 At The Eye Piece …..……………...……….….………………..….…. 8 The Cover Image - 47 Tuc and SMC ...…..…………..……..…….. 10 New General Catalogue …...………………………..…….…...….... 12 First Map Of Motion …...……………………………….…..………... 14 Three ISS Crew Return ………………………………….….……….. 16 James Webb Space Telescope vs Hubble …..………….….….... 18 Members Moments ……………….…………………………....…….. 22 The Month Ahead …..…………………...….…….……………..…… 24 Minutes Of The Meeting …………………………………………….. 25 Public Viewing Roster …………………………….……….…..……. 27 . ASSA Symposium 2018 ………………………...…………......…… 28 Member Submissions Disclaimer: The views expressed in ‘nDaba are solely those of the writer and are not necessarily the views of the Durban Centre, nor the Editor. All images and content is the work of the respective copyright owner Page 3 Chairman’s Chatter By Mike Hadlow Dear Members, The official start of spring with the Vernal Equinox occurred on 22 September 2017, so we are now officially into spring which is supposed to be start of our rainy season. So far it certainly has been a rainy start with very few clear viewing evenings being available. We were supposed to have a viewing at the Bluff Eco-Park on 16 September, but due to poor weather, cloud, rain and extremely high winds for the Durban area, this was cancelled. We nevertheless had a good representation at the eTthekwini Municipality’s sustainable living Expo and got the members of the public interested in astronomy by our professional display and through viewing through our telescopes focusing at models of Saturn and Jupiter hanging from the roof in the exhibition centre. -
ALABAMA University Libraries
THE UNIVERSITY OF ALABAMA University Libraries Seeing Galaxies through Thick and Thin. I. Optical Measures in Overlapping Galaxies Raymond E. White III – University of Alabama William C. Keel – University of Alabama Christopher J. Conselice – University of Chicago Deposited 09/18/2018 Citation of published version: White III, R., Keel, W., Conselice, C. (2000): Seeing Galaxies through Thick and Thin. I. Optical Measures in Overlapping Galaxies. The Astrophysical Journal, 542(2). DOI: https://doi.org/10.1086/317011 © 2000. The American Astronomical Society. All rights reserved. Printed in U.S.A. THE ASTROPHYSICAL JOURNAL, 542:761È778, 2000 October 20 ( 2000. The American Astronomical Society. All rights reserved. Printed in U.S.A. SEEING GALAXIES THROUGH THICK AND THIN. I. OPTICAL OPACITY MEASURES IN OVERLAPPING GALAXIES1 RAYMOND E. WHITE III2,3,4 NASA Goddard Space Flight Center, Laboratory for High Energy Astrophysics, Code 662, Greenbelt, MD 20771; and Department of Physics and Astronomy, University of Alabama, Tuscaloosa, AL 35487-0324 WILLIAM C. KEEL2,3,4 Department of Physics and Astronomy, University of Alabama, Tuscaloosa, AL 35487-0324 AND CHRISTOPHER J. CONSELICE3,5,6 Department of Astronomy and Astrophysics, University of Chicago, Chicago, IL 60637 Received 2000 April 28; accepted 2000 May 24 ABSTRACT We describe the use of partially overlapping galaxies to provide direct measurements of the e†ective absorption in galaxy disks, independent of assumptions about internal disk structure. The non- overlapping parts of the galaxies and symmetry considerations are used to reconstruct, via di†erential photometry, how much background galaxy light is lost in passing through the foreground disks. Exten- sive catalog searches and follow-up imaging yield D15È25 nearby galaxy pairs suitable for varying degrees of our analysis; 11 of the best such examples are presented here. -
5-6Index 6 MB
CLEAR SKIES OBSERVING GUIDES 5-6" Carbon Stars 228 Open Clusters 751 Globular Clusters 161 Nebulae 199 Dark Nebulae 139 Planetary Nebulae 105 Supernova Remnants 10 Galaxies 693 Asterisms 65 Other 4 Clear Skies Observing Guides - ©V.A. van Wulfen - clearskies.eu - [email protected] Index ANDROMEDA - the Princess ST Andromedae And CS SU Andromedae And CS VX Andromedae And CS AQ Andromedae And CS CGCS135 And CS UY Andromedae And CS NGC7686 And OC Alessi 22 And OC NGC752 And OC NGC956 And OC NGC7662 - "Blue Snowball Nebula" And PN NGC7640 And Gx NGC404 - "Mirach's Ghost" And Gx NGC891 - "Silver Sliver Galaxy" And Gx Messier 31 (NGC224) - "Andromeda Galaxy" And Gx Messier 32 (NGC221) And Gx Messier 110 (NGC205) And Gx "Golf Putter" And Ast ANTLIA - the Air Pump AB Antliae Ant CS U Antliae Ant CS Turner 5 Ant OC ESO435-09 Ant OC NGC2997 Ant Gx NGC3001 Ant Gx NGC3038 Ant Gx NGC3175 Ant Gx NGC3223 Ant Gx NGC3250 Ant Gx NGC3258 Ant Gx NGC3268 Ant Gx NGC3271 Ant Gx NGC3275 Ant Gx NGC3281 Ant Gx Streicher 8 - "Parabola" Ant Ast APUS - the Bird of Paradise U Apodis Aps CS IC4499 Aps GC NGC6101 Aps GC Henize 2-105 Aps PN Henize 2-131 Aps PN AQUARIUS - the Water Bearer Messier 72 (NGC6981) Aqr GC Messier 2 (NGC7089) Aqr GC NGC7492 Aqr GC NGC7009 - "Saturn Nebula" Aqr PN NGC7293 - "Helix Nebula" Aqr PN NGC7184 Aqr Gx NGC7377 Aqr Gx NGC7392 Aqr Gx NGC7585 (Arp 223) Aqr Gx NGC7606 Aqr Gx NGC7721 Aqr Gx NGC7727 (Arp 222) Aqr Gx NGC7723 Aqr Gx Messier 73 (NGC6994) Aqr Ast 14 Aquarii Group Aqr Ast 5-6" V2.4 Clear Skies Observing Guides - ©V.A. -
Arxiv:1905.10771V3 [Astro-Ph.HE] 28 May 2020 .S Ja .Ojha R
The Fourth Catalog of Active Galactic Nuclei Detected by the Fermi Large Area Telescope M. Ajello1, R. Angioni2,3, M. Axelsson4,5, J. Ballet6, G. Barbiellini7,8, D. Bastieri9,10, J. Becerra Gonzalez11, R. Bellazzini12, E. Bissaldi13,14, E. D. Bloom15, R. Bonino16,17, E. Bottacini18,15, P. Bruel19, S. Buson20, F. Cafardo21, R. A. Cameron15, E. Cavazzuti22, S. Chen9,18, C. C. Cheung23, S. Ciprini3,2,24, D. Costantin25, S. Cutini26, F. D’Ammando27, P. de la Torre Luque13, R. de Menezes21,17, F. de Palma16, A. Desai1, N. Di Lalla15, L. Di Venere13,14, A. Dom´ınguez28, F. Fana Dirirsa29, E. C. Ferrara30, J. Finke23, A. Franckowiak31, Y. Fukazawa32, S. Funk33, P. Fusco13,14, F. Gargano14, S. Garrappa31, D. Gasparrini3,2,34, N. Giglietto13,14, F. Giordano13,14, M. Giroletti27, D. Green35, I. A. Grenier6, S. Guiriec36,30, S. Harita37, E. Hays30, D. Horan19, R. Itoh38, G. J´ohannesson39,40, M. Kovac’evic’26, F. Krauss41, M. Kreter42,20, M. Kuss12, S. Larsson5,43,44, C. Leto2, J. Li31, I. Liodakis15, F. Longo7,8, F. Loparco13,14, B. Lott45,46, M. N. Lovellette23 , P. Lubrano26, G. M. Madejski15, S. Maldera16, A. Manfreda47, G. Mart´ı-Devesa48, F. Massaro17,16,49, M. N. Mazziotta14 , I.Mereu50,26, M. Meyer33, G. Migliori51,52, N. Mirabal30,53, T. Mizuno54, M. E. Monzani15, A. Morselli3, I. V. Moskalenko15, M. Negro55,53, R. Nemmen21, E. Nuss56, L. S. Ojha, R. Ojha30, N. Omodei15, M. Orienti27, E. Orlando57,15, J. F. Ormes58, V. S. Paliya31, Z. Pei10, H. Pe˜na-Herazo17,16,49,59,60, M.