Preliminary Catalogue of Isaac Roberts's Collection of Photographs of Celestial Objects
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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. -
The MUSE View of the Planetary Nebula NGC 3132? Ana Monreal-Ibero1,2 and Jeremy R
A&A 634, A47 (2020) Astronomy https://doi.org/10.1051/0004-6361/201936845 & © ESO 2020 Astrophysics The MUSE view of the planetary nebula NGC 3132? Ana Monreal-Ibero1,2 and Jeremy R. Walsh3,?? 1 Instituto de Astrofísica de Canarias (IAC), 38205 La Laguna, Tenerife, Spain e-mail: [email protected] 2 Universidad de La Laguna, Dpto. Astrofísica, 38206 La Laguna, Tenerife, Spain 3 European Southern Observatory, Karl-Schwarzschild Strasse 2, 85748 Garching, Germany Received 4 October 2019 / Accepted 6 December 2019 ABSTRACT Aims. Two-dimensional spectroscopic data for the whole extent of the NGC 3132 planetary nebula have been obtained. We deliver a reduced data-cube and high-quality maps on a spaxel-by-spaxel basis for the many emission lines falling within the Multi-Unit Spectroscopic Explorer (MUSE) spectral coverage over a range in surface brightness >1000. Physical diagnostics derived from the emission line images, opening up a variety of scientific applications, are discussed. Methods. Data were obtained during MUSE commissioning on the European Southern Observatory (ESO) Very Large Telescope and reduced with the standard ESO pipeline. Emission lines were fitted by Gaussian profiles. The dust extinction, electron densities, and temperatures of the ionised gas and abundances were determined using Python and PyNeb routines. 2 Results. The delivered datacube has a spatial size of 6300 12300, corresponding to 0:26 0:51 pc for the adopted distance, and ∼ × ∼ 1 × a contiguous wavelength coverage of 4750–9300 Å at a spectral sampling of 1.25 Å pix− . The nebula presents a complex reddening structure with high values (c(Hβ) 0:4) at the rim. -
Astronomy Magazine Special Issue
γ ι ζ γ δ α κ β κ ε γ β ρ ε ζ υ α φ ψ ω χ α π χ φ γ ω ο ι δ κ α ξ υ λ τ μ β α σ θ ε β σ δ γ ψ λ ω σ η ν θ Aι must-have for all stargazers η δ μ NEW EDITION! ζ λ β ε η κ NGC 6664 NGC 6539 ε τ μ NGC 6712 α υ δ ζ M26 ν NGC 6649 ψ Struve 2325 ζ ξ ATLAS χ α NGC 6604 ξ ο ν ν SCUTUM M16 of the γ SERP β NGC 6605 γ V450 ξ η υ η NGC 6645 M17 φ θ M18 ζ ρ ρ1 π Barnard 92 ο χ σ M25 M24 STARS M23 ν β κ All-in-one introduction ALL NEW MAPS WITH: to the night sky 42,000 more stars (87,000 plotted down to magnitude 8.5) AND 150+ more deep-sky objects (more than 1,200 total) The Eagle Nebula (M16) combines a dark nebula and a star cluster. In 100+ this intense region of star formation, “pillars” form at the boundaries spectacular between hot and cold gas. You’ll find this object on Map 14, a celestial portion of which lies above. photos PLUS: How to observe star clusters, nebulae, and galaxies AS2-CV0610.indd 1 6/10/10 4:17 PM NEW EDITION! AtlAs Tour the night sky of the The staff of Astronomy magazine decided to This atlas presents produce its first star atlas in 2006. -
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). -
Cetus - the Whale
May 18 2021 Cetus - The Whale Observed: No Object Her Type Mag Alias/Notes IC 5384 Non-Existent NGC 7813 MCG -2-1-16 MK 936 IRAS 15-1215 PGC 287 IC 1528 Non-Existent NGC 7826 H29-8 Non-Existent Asterism IC 1533 Non-Existent NGC 34 Non-Existent NGC 17 NGC 58 Non-Existent NGC 47 PGC 967 MCG -1-1-55 IRAS 119-726 NGC 54 Glxy SB(r)a? 14.6 MCG -1-1-60 PGC 1011 NGC 59 Glxy SA(rs)0-: 13.1 ESO 539-4 MCG -4-1-26 PGC 1034 NGC 62 Glxy (R)SB(r)a: 12.3 MCG -2-1-43 IRAS 145-1345 PGC 1125 NGC 64 Glxy SB(s)bc 14 MCG -1-1-68 IRAS 149-706 PGC 1149 IC 5 Glxy E 14.8 MCG -2-1-47 IRAS 148-951 PGC 1145 NGC 73 Glxy SAB(rs)bc: 13.5 MCG -3-1-26 PGC 1211 NGC 65 Glxy SAB(rs)0-: 14.4 ESO 473-10A MCG -4-2-1 PGC 1229 NGC 66 Glxy SB(r)b pec 14.2 ESO 473-10 MCG -4-2-2 IRAS 165-2312 PGC 1236 IC 9 Glxy Sb(r) 16.1 MCG -2-2-1 IRAS 171-1423 PGC 1271 NGC 77 Glxy SA0-: 15.7 ESO 473-15 PGC 1290 NGC 102 Glxy S0/a 14.4 MCG -2-2-11 PGC 1542 NGC 107 Glxy Sbc 14.6 MCG -2-2-14 PGC 1606 NGC 111 Non-Existent NGC 113 Glxy SA0-: 13.5 MCG -1-2-16 PGC 1656 NGC 114 Glxy SB(rs)0: 14.7 UGC 259 MCG 0-2-27 MK 946 CGCG 383-14 KUG 24-20A PGC 1660 NGC 116 Non-Existent MCG -1-2-17 PGC 1671 NGC 117 Glxy S0+: sp 15.3 MCG 0-2-29 CGCG 383-15 PGC 1674 NGC 118 Glxy I0? 14.8 UGC 264 MCG 0-2-32 MK 947 CGCG 383-16 UM244 3ZW9 IRAS 247-203 PGC 1678 NGC 120 Glxy SB0^: 14.4 UGC 267 MCG 0-2-33 CGCG 383-17 PGC 1693 NGC 122 Non-Existent NGC 123 Non-Existent NGC 124 Glxy SA(s)c 13.7 UGC 271 MCG 0-2-38 CGCG 383-18 IRAS 253-205 PGC 1715 IC 15 Non-Existent IC 16 Glxy E? 14.7 MCG -2-2-17 IRAS 255-1322 PGC 1730 IC 17 -
Stars and Their Purpose
Stars & Their Purpose.indd 3 8/17/06 8:19:54 AM First Master Books printing: August 2006 Copyright © 2006 by Werner Gitt. All rights reserved. No part of this book may be used or reproduced in any manner whatsoever without written permission of the publisher except in the case of brief quotations in articles and reviews. For information write: Master Books, P.O. Box 726, Green Forest, AR 72638. ISBN-13: 978-0-89051-482-5 ISBN-10: 0-89051-482-8 Library of Congress Number: 2006929548 Cover by Bryan Miller Unless otherwise noted, all Scripture is from the New International Version of the Bible. References to apocryphal books have been taken from The Jerusalem Bible (London: Darton, Longman & Todd, 1966 edition). Printed in the United States of America. Please visit our website for other great titles: www.masterbooks.net. For information regarding author interviews, please contact the publicity department at (870) 528-5288. Stars & Their Purpose.indd 4 8/17/06 8:19:54 AM INDEX Preface............................................................................. 7 Preface to the English Edition ....................................... 13 Introduction.................................................................. 15 1. Can the Stars Be Counted?............................................ 17 2. In What Respects Do the Stars Differ?........................... 27 3. How Big Is the Universe? .............................................. 39 4. Four Characteristics of Space......................................... 43 5. Why Were the Stars Created? ........................................ 49 5.1 The Stars Were Made to Shine on Earth................. 50 5.2 The Stars Were Made to Determine Times and Seasons ................................................. 53 6. How Do the Stars Transmit Their Messages? ................. 57 6.1 Their Messages Are Silent....................................... 57 6.2 God’s Message Can Be Understood by Anybody ... -
SAC's 110 Best of the NGC
SAC's 110 Best of the NGC by Paul Dickson Version: 1.4 | March 26, 1997 Copyright °c 1996, by Paul Dickson. All rights reserved If you purchased this book from Paul Dickson directly, please ignore this form. I already have most of this information. Why Should You Register This Book? Please register your copy of this book. I have done two book, SAC's 110 Best of the NGC and the Messier Logbook. In the works for late 1997 is a four volume set for the Herschel 400. q I am a beginner and I bought this book to get start with deep-sky observing. q I am an intermediate observer. I bought this book to observe these objects again. q I am an advance observer. I bought this book to add to my collect and/or re-observe these objects again. The book I'm registering is: q SAC's 110 Best of the NGC q Messier Logbook q I would like to purchase a copy of Herschel 400 book when it becomes available. Club Name: __________________________________________ Your Name: __________________________________________ Address: ____________________________________________ City: __________________ State: ____ Zip Code: _________ Mail this to: or E-mail it to: Paul Dickson 7714 N 36th Ave [email protected] Phoenix, AZ 85051-6401 After Observing the Messier Catalog, Try this Observing List: SAC's 110 Best of the NGC [email protected] http://www.seds.org/pub/info/newsletters/sacnews/html/sac.110.best.ngc.html SAC's 110 Best of the NGC is an observing list of some of the best objects after those in the Messier Catalog. -
Open Clusters
Open Clusters Open clusters (also known as galactic clusters) are of tremendous importance to the science of astronomy, if not to astrophysics and cosmology generally. Star clusters serve as the "laboratories" of astronomy, with stars now all at nearly the same distance and all created at essentially the same time. Each cluster thus is a running experiment, where we can observe the effects of composition, age, and environment. We are hobbled by seeing only a snapshot in time of each cluster, but taken collectively we can understand their evolution, and that of their included stars. These clusters are also important tracers of the Milky Way and other parent galaxies. They help us to understand their current structure and derive theories of the creation and evolution of galaxies. Just as importantly, starting from just the Hyades and the Pleiades, and then going to more distance clusters, open clusters serve to define the distance scale of the Milky Way, and from there all other galaxies and the entire universe. However, there is far more to the study of star clusters than that. Anyone who has looked at a cluster through a telescope or binoculars has realized that these are objects of immense beauty and symmetry. Whether a cluster like the Pleiades seen with delicate beauty with the unaided eye or in a small telescope or binoculars, or a cluster like NGC 7789 whose thousands of stars are seen with overpowering wonder in a large telescope, open clusters can only bring awe and amazement to the viewer. These sights are available to all. -
Alma Observations of Warm Molecular Gas and Cold Dust in Ngc 34∗
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by Caltech Authors The Astrophysical Journal, 787:48 (10pp), 2014 May 20 doi:10.1088/0004-637X/787/1/48 C 2014. The American Astronomical Society. All rights reserved. Printed in the U.S.A. ALMA OBSERVATIONS OF WARM MOLECULAR GAS AND COLD DUST IN NGC 34∗ C. K. Xu1,C.Cao1,2,3,N.Lu1,Y.Gao4, P. van der Werf5,A.S.Evans6,7, J. M. Mazzarella1, J. Chu8,S.Haan9, T. Diaz-Santos1, R. Meijerink5, Y.-H. Zhao1,4, P. Appleton1, L. Armus1, V. Charmandaris10,11,12,S.Lord1, E. J. Murphy1, D. B. Sanders8, B. Schulz1, and S. Stierwalt6,13 1 Infrared Processing and Analysis Center, MS 100-22, California Institute of Technology, Pasadena, CA 91125, USA 2 School of Space Science and Physics, Shandong University at Weihai, Weihai, Shandong 264209, China; [email protected] 3 Shandong Provincial Key Laboratory of Optical Astronomy and Solar-Terrestrial Environment, Weihai, Shandong 264209, China 4 Purple Mountain Observatory, Chinese Academy of Sciences, 2 West Beijing Road, Nanjing 210008, China 5 Leiden Observatory, Leiden University, P.O. Box 9513, NL-2300 RA Leiden, Netherlands 6 Department of Astronomy, University of Virginia, P.O. Box 400325, Charlottesville, VA 22904, USA 7 National Radio Astronomy Observatory, Charlottesville, VA 22904, USA 8 Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI 96816, USA 9 CSIRO Astronomy and Space Science, ATNF, P.O. Box 76, Epping 1710, Australia 10 Department of Physics, University of Crete, GR-71003, Heraklion, Greece 11 Institute for Astronomy, Astrophysics, Space Applications & Remote Sensing, National Observatory of Athens, GR-15236, Penteli, Greece 12 Chercheur Associe,´ Observatoire de Paris, F-75014, Paris, France 13 Spitzer Science Center, California Institute of Technology, 1200 E. -
Just What Are Those Sky Chart "M" and "NGC" Numbers? by Barry D
Just what are those Sky Chart "M" and "NGC" Numbers? By Barry D. Malpas – Special to the Williams-Grand Canyon News – 2014 November One of the pastimes for some early sky observers was to locate new comets. Charles Messier (1730-1817) was a French comet hunter during the late 1700s, and discovered 13 new comets between 1760 and 1785. His interest in astronomy, and comets in particular, was influenced by seeing the great comet of 1744, and the comet of 1759 (of which Edmond Halley had believed the comets of 1531, 1607, and 1682 were the same and had predicted the comet’s 1759 apparition which is now known as Halley's Comet.) At this time telescopes were relatively small. The understanding of supernovae, or galaxies, was not yet in the current knowledge, as such objects only appeared as blurry smudges that did not move across the sky. In order not to waste time and become frustrated with viewing fuzzy objects that resembled, but were not, comets, Messier compiled a list of 110 of these celestial blurs which we now refer to as Messier, or "M Objects." The Messier Catalog has become a very popular list of "Deep Sky Objects" among amateur astronomers around the world because it consists of most of the galaxies, nebulae and star clusters easily observable with binoculars or small telescopes in the northern skies. Now, however, the objects in the list are the source of interest, as opposed to the reason the compilation was originally intended by Messier. At large astronomical get-togethers, known as "star parties", there is often a "Messier Marathon" competition to view the most Messier Objects during one observing night. -
SAA 100 Club
S.A.A. 100 Observing Club Raleigh Astronomy Club Version 1.2 07-AUG-2005 Introduction Welcome to the S.A.A. 100 Observing Club! This list started on the USENET newsgroup sci.astro.amateur when someone asked about everyone’s favorite, non-Messier objects for medium sized telescopes (8-12”). The members of the group nominated objects and voted for their favorites. The top 100 objects, by number of votes, were collected and ranked into a list that was published. This list is a good next step for someone who has observed all the objects on the Messier list. Since it includes objects in both the Northern and Southern Hemispheres (DEC +72 to -72), the award has two different levels to accommodate those observers who aren't able to travel. The first level, the Silver SAA 100 award requires 88 objects (all visible from North Carolina). The Gold SAA 100 Award requires all 100 objects to be observed. One further note, many of these objects are on other observing lists, especially Patrick Moore's Caldwell list. For convenience, there is a table mapping various SAA100 objects with their Caldwell counterparts. This will facilitate observers who are working or have worked on these lists of objects. We hope you enjoy looking at all the great objects recommended by other avid astronomers! Rules In order to earn the Silver certificate for the program, the applicant must meet the following qualifications: 1. Be a member in good standing of the Raleigh Astronomy Club. 2. Observe 80 Silver observations. 3. Record the time and date of each observation. -
Caldwell Catalogue - Wikipedia, the Free Encyclopedia
Caldwell catalogue - Wikipedia, the free encyclopedia Log in / create account Article Discussion Read Edit View history Caldwell catalogue From Wikipedia, the free encyclopedia Main page Contents The Caldwell Catalogue is an astronomical catalog of 109 bright star clusters, nebulae, and galaxies for observation by amateur astronomers. The list was compiled Featured content by Sir Patrick Caldwell-Moore, better known as Patrick Moore, as a complement to the Messier Catalogue. Current events The Messier Catalogue is used frequently by amateur astronomers as a list of interesting deep-sky objects for observations, but Moore noted that the list did not include Random article many of the sky's brightest deep-sky objects, including the Hyades, the Double Cluster (NGC 869 and NGC 884), and NGC 253. Moreover, Moore observed that the Donate to Wikipedia Messier Catalogue, which was compiled based on observations in the Northern Hemisphere, excluded bright deep-sky objects visible in the Southern Hemisphere such [1][2] Interaction as Omega Centauri, Centaurus A, the Jewel Box, and 47 Tucanae. He quickly compiled a list of 109 objects (to match the number of objects in the Messier [3] Help Catalogue) and published it in Sky & Telescope in December 1995. About Wikipedia Since its publication, the catalogue has grown in popularity and usage within the amateur astronomical community. Small compilation errors in the original 1995 version Community portal of the list have since been corrected. Unusually, Moore used one of his surnames to name the list, and the catalogue adopts "C" numbers to rename objects with more Recent changes common designations.[4] Contact Wikipedia As stated above, the list was compiled from objects already identified by professional astronomers and commonly observed by amateur astronomers.