A Glimpse Into the Life of Charles Messier 1

Total Page:16

File Type:pdf, Size:1020Kb

A Glimpse Into the Life of Charles Messier 1 Cambridge University Press 978-1-107-01837-2 - Deep-Sky Companions: The Messier Objects: Second Edition Stephen James O’Meara Excerpt More information CHAPTER 1 A glimpse into the life of 1 Charles Messier had no time to check the positions of M é chain’s additions, he added them to his list, bring- ing to 103 the total num- ber of nebulae and star clusters in it. Th is fi nal compendium (the last to be created by Messier) appeared in the French almanac Connaissance des Temps for 1784 (pub- lished in 1781). Th e number of objects in Messier’s catalogue has since increased to 110: the original 103 objects, plus 7 more added posthumously by other astronomers for various reasons. (I will discuss these latter objects in more detail later.) In recent times, we have also learned that object number 102 in Messier’s 1781 list may CCharlesharles MMessieressier be a duplicate obser- vation of object num- ber 101; but this matter On the evening of April 13, 1781, French remains a topic of much interesting debate. astronomer Charles Messier (1730–1817) Regardless, the 103 objects in Messier’s cata- made his fi nal observation for what was to logue and the seven subsequent additions become the most extensive catalogue of neb- have endured the test of time to become ulae and star clusters of the time. Th e list, the most popular listing of deep-sky objects which took more than two decades to create, targeted by Northern Hemisphere amateur contained the positions and descriptions of astronomers (both visual and astro-imagers 100 objects visible above his Paris horizon alike), especially by those just beginning in (48 ° 51′ north). Just before Messier submitted the hobby. this list for publication, he received from his Ironically, this was not Messier’s intent. contemporary Pierre M é chain (1744–1804) a “What caused me to undertake the catalogue,” note that included information on three more Messier explained in the Connaissance des objects discovered by him. Although Messier Temps for 1801, “was the nebula I discovered A glimpse into the life of Charles Messier 1 © in this web service Cambridge University Press www.cambridge.org Cambridge University Press 978-1-107-01837-2 - Deep-Sky Companions: The Messier Objects: Second Edition Stephen James O’Meara Excerpt More information 1 above the southern horn of Taurus on dixhuitième Siècle [History of Astronomy in the September 12, 1758, while observing the Eighteenth Century], by Delambre. La Harpe comet for that year.… Th is nebula had such ( Correspondence Litteraire , Paris, 1801, tom. a resemblance to a comet, in its form and i, p. 97) says that “he passed his life in search brightness, that I endeavored to fi nd others, of comets. Th e ne plus ultra of his ambition was to be made a member of the Academy of so that astronomers would not confuse these Petersburgh. He was an excellent man, but same nebulae with comets just beginning to had the simplicity of a child. At a time when he shine … and this is the purpose I had in form- was in expectation of discovering a comet, his ing the catalogue.” wife took ill and died. While attending upon Messier, the fi rst astronomer to devote her, being withdrawn from his observatory, himself to the systematic search for comets, Montaigne de Limoges anticipated him by dis- had obviously suff ered the frustration of wast- covering the comet. Messier was in despair. A ing time on “false comets” – diff use deep-sky friend visiting him began to off er some conso- objects that could be mistaken for comets lation for the recent affl iction he had suff ered. during a sweep of the heavens, especially with Messier, thinking only of his comet, exclaimed: – a small telescope at low power; every minute ‘I had discovered twelve. Alas, that I should be spent on a “false” comet was time spent away robbed of the thirteenth by Montaigne!’ and his eyes fi lled with tears. Th en, remembering that from the potential discovery of a real one in it was necessary to mourn for his wife, whose this highly competitive pursuit. remains were still in the house, he exclaimed, – Unlike the skywatchers of today, Messier ‘Ah! cette pauvre femme , ’ [Ah! Th is poor woman] had no star charts with known deep-sky and again wept for his comet.” objects plotted on them, except for a few that included some of the brightest naked- THE “BIRD-NESTER” OF COMETS eye wonders, such as the Beehive (M44) or Given the incredible and effi cient technolo- Pleiades (M45) star clusters. To further his gies used to discover comets in the twenty- success, one could say Messier employed fi rst century, both on Earth and in space, the intelligent strategy of “knowing thy many of today’s telescopic observers pursue enemy”: the objects Messier included in comets mostly as objects of passing interest – his catalogue are those he wanted to know especially when they blaze forth to naked-eye existed, so that he could ignore them and splendor or threaten to hit the Earth … or move along in his attempt to visually capture other planets! (Note, however, that owing to his ultimate prey. the same leaps in technology, some amateur Th e magnitude to which Messier was per- astronomers across the globe also conduct ceived to dedicate his thoughts to the hunt extremely serious studies of, and searches is refl ected in a colorful story that has been for, comets, and have contributed greatly to passed down since the beginning of the nine- the science.) Nevertheless, to the mid-eigh- teenth century. Here is the tale, as told by teenth-century observer, comets were among French astronomer Fran ç ois Arago (1786– the most mystifying sights in the sky. And the 1853) in his Popular Lectures on Astronomy: astonishing appearance of six-tailed C/1743 Delivered at the Royal Observatory of Paris , XI (Ché seaux’s comet of 1744) – one of the published in 1845: greatest since the dawn of modern astron- An interesting memoir of Messier may be omy – may have inspired Messier’s lifelong found in the Histoire de l‘Astronomie au passion for comets. 2 Deep-Sky Companions: The Messier Objects © in this web service Cambridge University Press www.cambridge.org Cambridge University Press 978-1-107-01837-2 - Deep-Sky Companions: The Messier Objects: Second Edition Stephen James O’Meara Excerpt More information 1 his brother’s personal clerk, Charles obtained the skills of clean hand- writing, draftsmanship, and journal keeping – all traits that would soon help him secure his future employment at the Paris Observatory. Charles led a safe and secure country life, immersing himself in his spare time in the natural wonders of the local countryside. He also grew up during the height of Rococo devel- opment in France, the CCometomet C/2006C/2006 P1P1 ((McNaught).McNaught). start of the classical period of music, and With history having recorded only some 50 the time of the cultural Enlightenment in comets known by Messier’s time, these celes- Europe. Th ese important shifts in scientifi c tial itinerants presented the burgeoning tele- and cultural trends may have swept up young scopic astronomers of the day not only with Messier’s thoughts in their currents, leading a fascinating challenge (namely to fi nd them) him into new areas of imagining. And while but also the promise of some fame and notori- it is uncertain what exactly inspired Messier’s ety. And Messier was the man who fi rst thrust interest in astronomy, the remarkable sight this challenge to the forefront of desire. of Ch é seaux’s comet in 1744 and the annu- Messier was born on June 26, 1730, in the lar solar eclipse of June 25, 1748 (visible small village of Badouvillier, Lorraine (about from his hometown), must have been major 200 miles east of Paris, near the German bor- infl uences. der). He was the tenth of 12 children born to When a changing political climate in Nicolas and Francoise Messier, and one of France in 1751 forced his brother Hyacinthe only six to survive into adulthood. His father to take a position as a tax collector in his was a type of mayor/administrator, who, mother’s hometown, the orphaned Charles among other duties, collected taxes through- found himself in need of a job. With the help out the serfdom and served as a judge for of a family friend, Charles traveled to Paris local misdemeanors; Nicolas passed away in that October to meet with astronomer Joseph 1741, when Charles was only 11. Nicolas Delisle, who then hired Messier to be When Charles’s older brother Hyacinthe his apprentice at the Marine Observatory at took over the Messier household, he began to the Hotel de Cluny in Paris – even though, as prep young Charles as a manager of fi nances – Delisle said, the young man had “hardly any Hyacinthe’s particular fi eld of expertise. As other recommendation than that of a neat A glimpse into the life of Charles Messier 3 © in this web service Cambridge University Press www.cambridge.org Cambridge University Press 978-1-107-01837-2 - Deep-Sky Companions: The Messier Objects: Second Edition Stephen James O’Meara Excerpt More information 1 and legible handwriting and some little abil- Messier’s comet pursuits blossomed after ity in draughtsmanship.” Delisle retired in 1761, the year Messier took Nevertheless, Delisle assigned Messier the charge of the observatory, observed the transit task of mapmaking and the recording of astro- of Venus, and made other acute observations.
Recommended publications
  • Optical Astronomy Catalogues, Coordinates Visible Objects on the Sky • Stars • Planets • Comets & Asteroids • Nebulae & Galaxies
    Astrophysics Content: 2+2, 2×13×90 = 2 340 minutes = 39 hours Tutor: Martin Žáček [email protected] department of Physics, room 49 On-line informations: http://fyzika.feld.cvut.cz/~zacek/ … this presentation Many years (20?) teaching astrophysics (Prof. Petr Kulhanek), many texts and other materials but mostly in Czech (for example electronic journal Aldebaran Bulletin). 2011 … first year of teaching Astrophysics in English 2012-16 … 2017 … about 6 students, lextures on Thursday 11:00 lecture and 12:45 exercise https://www.fel.cvut.cz/cz/education/bk/predmety/12/77/p12773704.html ... AE0B02ASF https://www.fel.cvut.cz/cz/education/bk/predmety/12/78/p12784304.html ... AE0M02ASF Syllabus Classes: Astronomy & astrophysics 1. Astrophysics, history and its place in context of natural sciences. 2. Foundations of astronomy, history, its methods, instruments. 3. Solar system, inner and outer planets, Astronomical coordinates. Physics of stars 4. Statistics of stars, HR diagram. The star formation and evolution. Hyashi line. 5. Final evolutionary stages. White dwarfs, neutron stars, black holes. 6. Variable stars. Cepheids. Novae and supernovae stars. Binary systems. 7. Other galactic and extragalactic objects, nebulae, star clusters, galaxies. Cosmology 8. Principle of special and general theory of relativity. Relativistic experiments. 9. Cosmology. The Universe evolution, cosmological principle. Friedman models. 10. Supernovae Ia, cosmological parameters of the Universe, dark matter and dark energy. 11. Elementary particles, fundamental forces, quantum field theory, Feynman diagrams. 12. The origin of the Universe. Quark-gluon plasma. Nucleosynthesis. Microwave background radiation. 13. Cosmology with the inflationary phase, long-scale structure of the Universe. 14. Reserve Syllabus Practices: Astronomy & astrophysics 1.
    [Show full text]
  • Winter Messier List Observing Club
    Winter Messier List Observing Club Raleigh Astronomy Club Version 1.1 24 November 2012 Introduction Welcome to the Winter Messier List Observing Club. The objects on this list represent many of the most prominent deep sky objects (Globular Clusters, Open Clusters, Nebula, Galaxies) visible from mid-northern latitudes. The Messier list of objects was compiled in the 1700’s by the French comet hunter Charles Messier and his associates as a list of objects to not confuse with their primary goal of discovering new comets. What they really produced, was a list of many of the best deep sky objects for astronomers to enjoy. Observing the Messier List is an excellent way for beginning astronomers to learn the night sky. This club is intended for those who wish to tour the Messier objects while adding more structure to their observing activities. Club members who wish to work their way through the Messier objects, a season at a time, will find this list to be a helpful guide. Two certificate levels are offered, Silver and Gold. The Silver certificate is earned by viewing and logging all objects on the list while using Go-To or Digital Setting Circles to help locate the Messier objects. The Gold certificate is earned by those who view and log all the objects while only using charts and star hopping to locate them. Anyone who intends to use their RAC list results as a stepping-stone to the Astronomlcal League Messier certificate, MUST work to the Gold certificate rules. Rules To earn the Winter Messier List certificate, you must: 1.
    [Show full text]
  • 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.
    [Show full text]
  • 1 the Comets of Caroline Herschel (1750-1848)
    Inspiration of Astronomical Phenomena, INSAP7, Bath, 2010 (www.insap.org) 1 publication: Culture and Cosmos, Vol. 16, nos. 1 and 2, 2012 The Comets of Caroline Herschel (1750-1848), Sleuth of the Skies at Slough Roberta J. M. Olson1 and Jay M. Pasachoff2 1The New-York Historical Society, New York, NY, USA 2Hopkins Observatory, Williams College, Williamstown, MA, USA Abstract. In this paper, we discuss the work on comets of Caroline Herschel, the first female comet-hunter. After leaving Bath for the environs of Windsor Castle and eventually Slough, she discovered at least eight comets, five of which were reported in the Philosophical Transactions of the Royal Society. We consider her public image, astronomers' perceptions of her contributions, and the style of her astronomical drawings that changed with the technological developments in astronomical illustration. 1. General Introduction and the Herschels at Bath Building on the research of Michael Hoskini and our book on comets and meteors in British art,ii we examine the comets of Caroline Herschel (1750-1848), the first female comet-hunter and the first salaried female astronomer (Figure 1), who was more famous for her work on nebulae. She and her brother William revolutionized the conception of the universe from a Newtonian one—i.e., mechanical with God as the great clockmaker watching over its movements—to a more modern view—i.e., evolutionary. Figure 1. Silhouette of Caroline Herschel, c. 1768, MS. Gunther 36, fol. 146r © By permission of the Oxford University Museum of the History of Science Inspiration of Astronomical Phenomena, INSAP7, Bath, 2010 (www.insap.org) 2 publication: Culture and Cosmos, Vol.
    [Show full text]
  • Alexandre Amorim -.:: GEOCITIES.Ws
    Alexandre Amorim (org) 2 3 PREFÁCIO O Boletim Observe! é uma iniciativa da Coordenação de Observação Astronômica do Núcleo de Estudo e Observação Astronômica “José Brazilício de Souza” (NEOA-JBS). Durante a reunião administrativa do NEOA-JBS em maio de 2010 foi apresentada a edição de Junho de 2010 para apreciação dos demais coordenadores do Núcleo onde houve aprovação unânime em usar o Boletim Observe! como veículo de informação das atividades e, principalmente, observações astronômicas. O Boletim Observe! é publicado mensalmente em formato eletrônico ou impresso separadamente, prezando pela simplicidade das informações e encorajando os leitores a observar, registrar e publicar os eventos astronômicos. Desde a sua primeira edição o Boletim Observe! conta com a colaboração espontânea de diversos astrônomos amadores e profissionais. Toda edição do Observe! do mês de dezembro é publicado um índice dos artigos do respectivo ano. Porém, desde aquela edição de Junho de 2010 foram publicados centenas de artigos e faz-se necessário consultar assuntos que foram tratados nas edições anteriores do Observe! e seus respectivos autores. Para isso publicaremos anualmente esse Índice de Assuntos, permitindo a consulta rápida dos temas abordados. Florianópolis, 1º de dezembro de 2018 Alexandre Amorim Coordenação de Observação Astronômica do NEOA-JBS 4 Ano I (2010) Nº 1 – Junho 2010 Eclipse da Lua em 26 de junho de 2010 Amorim, A. Júpiter sem a Banda Equatorial Sul Amorim, A. Conjunção entre Júpiter e Urano Amorim, A. Causos do Avelino Alves, A. A. Quem foi Eugênia de Bessa? Amorim, A. Nº 2 – Julho 2010 Aprendendo a dimensionar as distâncias angulares no céu Neves, M.
    [Show full text]
  • OCTOBER 2011 Next Meeting
    PRET ORI A CENT RE ASSA - OCT OBER 2011 PAGE 1 NEWSLETTER OCTOBER 2011 Next meeting Venue: The auditorium behind the main building at Christian Brothers College (CBC), Mount Edmund, Pretoria Road, Silverton, Pretoria. Date and time: Wednesday 26 October at 19h15. Programme: • Beginner’s Corner: "Introduction to spectroscopy" by Tom Field. (See bottom of page 10 of this newsletter.) • What’s Up? by Danie Barnardo. • 10 minute break — library will be open. • Main talk: "Destination Moon" by Patricia Skelton. • Socializing over tea/coffee and biscuits. The chairperson at the meeting will be Pat Kühn. Next observing evening: Friday 21 October at the Pretoria Centre Observatory, which is also situated at CBC. Turn left immediately after entering the main gate and follow the road. Arrive from sunset onwards. CONTENTS OF THIS NEWSLETTER Chairman's report of last month’s meeting 2 Solar eclipse series 2 Last month’s observing evening 3 The Crab Nebula viewing season Is almost upon us 4 Photographing the Moon’s parallax 5 Summary of “What’s Up?” to be presented on 26 October 6 For the Pretoria ASSA Deep Sky Observers (or any observer) 7 Feature of the month: Comet Elenin 8 News items 9 Basics: The blink comparator 10 Note about “Beginner’s Corner” on 26 October 10 Arp 273 - two interacting galaxies 11 Pretoria Centre committee 11 PAGE 2 PRET ORI A CENT RE ASSA - OCT OBER 2011 Chairman's report of last month’s meeting Beginner’s corner featured a fascinating presentation which amounted to an exposition of astronomical sleuthing by James Thomas.
    [Show full text]
  • Structure, Properties and Formation Histories of S0 Galaxies
    Structure, Properties and Formation Histories of S0 Galaxies by Kaustubh Vaghmare Thesis Supervisor Prof. Ajit K. Kembhavi A thesis presented for the degree of Doctor of Philosophy to IUCAA & Jawaharlal Nehru University India July, 2015 Structure, Properties and Formation Histories of S0 Galaxies by Kaustubh Vaghmare c 2015 All rights reserved. Certificate This is to certify that the thesis entitled Structure, Properties and Formation Histories of S0 Galaxies submitted by Mr. Kaustubh Vaghmare for the award of the degree of Doctor of Philosophy to Jawaharlal Nehru University, New Delhi is his original work. This has not been published or submitted to any other University for any other Degree or Diploma. Pune July 30th, 2015 Prof. Ajit K. Kembhavi (Thesis Advisor & Director, IUCAA) Declaration I hereby declare that the work reported in this thesis is entirely original. This thesis is composed independently by me at the Inter-University Centre for Astronomy and Astrophysics, Pune under the supervision of Prof. Ajit K. Kembhavi. I further declare that the subject matter presented in the thesis has not previously formed the basis for the award of any degree, diploma, associateship, fellowship or any other similar title of any University or Institution. Pune July 30th, 2015 Prof. Ajit K. Kembhavi Mr. Kaustubh Vaghmare (Thesis Advisor) (Ph.D. Candidate) 3 Dedicated to ... Prathama & Prakash (my parents, my Gods) Rahul (my brother, whose ever presence with my parents and unquestioning support allowed me to work in peace) & Sneha (my beloved) 5 Acknowledgements For all students and regular visitors, it is clear that Prof. Ajit Kembhavi is one of the busiest people with frequent meetings, visits abroad, directorial duties and several other responsibilities.
    [Show full text]
  • And Ecclesiastical Cosmology
    GSJ: VOLUME 6, ISSUE 3, MARCH 2018 101 GSJ: Volume 6, Issue 3, March 2018, Online: ISSN 2320-9186 www.globalscientificjournal.com DEMOLITION HUBBLE'S LAW, BIG BANG THE BASIS OF "MODERN" AND ECCLESIASTICAL COSMOLOGY Author: Weitter Duckss (Slavko Sedic) Zadar Croatia Pусскй Croatian „If two objects are represented by ball bearings and space-time by the stretching of a rubber sheet, the Doppler effect is caused by the rolling of ball bearings over the rubber sheet in order to achieve a particular motion. A cosmological red shift occurs when ball bearings get stuck on the sheet, which is stretched.“ Wikipedia OK, let's check that on our local group of galaxies (the table from my article „Where did the blue spectral shift inside the universe come from?“) galaxies, local groups Redshift km/s Blueshift km/s Sextans B (4.44 ± 0.23 Mly) 300 ± 0 Sextans A 324 ± 2 NGC 3109 403 ± 1 Tucana Dwarf 130 ± ? Leo I 285 ± 2 NGC 6822 -57 ± 2 Andromeda Galaxy -301 ± 1 Leo II (about 690,000 ly) 79 ± 1 Phoenix Dwarf 60 ± 30 SagDIG -79 ± 1 Aquarius Dwarf -141 ± 2 Wolf–Lundmark–Melotte -122 ± 2 Pisces Dwarf -287 ± 0 Antlia Dwarf 362 ± 0 Leo A 0.000067 (z) Pegasus Dwarf Spheroidal -354 ± 3 IC 10 -348 ± 1 NGC 185 -202 ± 3 Canes Venatici I ~ 31 GSJ© 2018 www.globalscientificjournal.com GSJ: VOLUME 6, ISSUE 3, MARCH 2018 102 Andromeda III -351 ± 9 Andromeda II -188 ± 3 Triangulum Galaxy -179 ± 3 Messier 110 -241 ± 3 NGC 147 (2.53 ± 0.11 Mly) -193 ± 3 Small Magellanic Cloud 0.000527 Large Magellanic Cloud - - M32 -200 ± 6 NGC 205 -241 ± 3 IC 1613 -234 ± 1 Carina Dwarf 230 ± 60 Sextans Dwarf 224 ± 2 Ursa Minor Dwarf (200 ± 30 kly) -247 ± 1 Draco Dwarf -292 ± 21 Cassiopeia Dwarf -307 ± 2 Ursa Major II Dwarf - 116 Leo IV 130 Leo V ( 585 kly) 173 Leo T -60 Bootes II -120 Pegasus Dwarf -183 ± 0 Sculptor Dwarf 110 ± 1 Etc.
    [Show full text]
  • The Comet's Tale
    THE COMET’S TALE Journal of the Comet Section of the British Astronomical Association Number 33, 2014 January Not the Comet of the Century 2013 R1 (Lovejoy) imaged by Damian Peach on 2013 December 24 using 106mm F5. STL-11k. LRGB. L: 7x2mins. RGB: 1x2mins. Today’s images of bright binocular comets rival drawings of Great Comets of the nineteenth century. Rather predictably the expected comet of the century Contents failed to materialise, however several of the other comets mentioned in the last issue, together with the Comet Section contacts 2 additional surprise shown above, put on good From the Director 2 appearances. 2011 L4 (PanSTARRS), 2012 F6 From the Secretary 3 (Lemmon), 2012 S1 (ISON) and 2013 R1 (Lovejoy) all Tales from the past 5 th became brighter than 6 magnitude and 2P/Encke, 2012 RAS meeting report 6 K5 (LINEAR), 2012 L2 (LINEAR), 2012 T5 (Bressi), Comet Section meeting report 9 2012 V2 (LINEAR), 2012 X1 (LINEAR), and 2013 V3 SPA meeting - Rob McNaught 13 (Nevski) were all binocular objects. Whether 2014 will Professional tales 14 bring such riches remains to be seen, but three comets The Legacy of Comet Hunters 16 are predicted to come within binocular range and we Project Alcock update 21 can hope for some new discoveries. We should get Review of observations 23 some spectacular close-up images of 67P/Churyumov- Prospects for 2014 44 Gerasimenko from the Rosetta spacecraft. BAA COMET SECTION NEWSLETTER 2 THE COMET’S TALE Comet Section contacts Director: Jonathan Shanklin, 11 City Road, CAMBRIDGE. CB1 1DP England. Phone: (+44) (0)1223 571250 (H) or (+44) (0)1223 221482 (W) Fax: (+44) (0)1223 221279 (W) E-Mail: [email protected] or [email protected] WWW page : http://www.ast.cam.ac.uk/~jds/ Assistant Director (Observations): Guy Hurst, 16 Westminster Close, Kempshott Rise, BASINGSTOKE, Hampshire.
    [Show full text]
  • Classification of Galaxies Using Fractal Dimensions
    UNLV Retrospective Theses & Dissertations 1-1-1999 Classification of galaxies using fractal dimensions Sandip G Thanki University of Nevada, Las Vegas Follow this and additional works at: https://digitalscholarship.unlv.edu/rtds Repository Citation Thanki, Sandip G, "Classification of galaxies using fractal dimensions" (1999). UNLV Retrospective Theses & Dissertations. 1050. http://dx.doi.org/10.25669/8msa-x9b8 This Thesis is protected by copyright and/or related rights. It has been brought to you by Digital Scholarship@UNLV with permission from the rights-holder(s). You are free to use this Thesis in any way that is permitted by the copyright and related rights legislation that applies to your use. For other uses you need to obtain permission from the rights-holder(s) directly, unless additional rights are indicated by a Creative Commons license in the record and/ or on the work itself. This Thesis has been accepted for inclusion in UNLV Retrospective Theses & Dissertations by an authorized administrator of Digital Scholarship@UNLV. For more information, please contact [email protected]. INFORMATION TO USERS This manuscript has been reproduced from the microfilm master. UMI films the text directly from the original or copy submitted. Thus, some thesis and dissertation copies are in typewriter face, while others may be from any type of computer printer. The quality of this reproduction is dependent upon the quality of the copy submitted. Broken or indistinct print, colored or poor quality illustrations and photographs, print bleedthrough, substandard margins, and improper alignment can adversely affect reproduction. In the unlikely event that the author did not send UMI a complete manuscript and there are missing pages, these will be noted.
    [Show full text]
  • An Ultra-Deep Survey of Low Surface Brightness Galaxies in Virgo
    ' $ An Ultra-Deep Survey of Low Surface Brightness Galaxies in Virgo Elizabeth Helen (Lesa) Moore, BSc(Hons) Department of Physics Macquarie University May 2008 This thesis is presented for the degree of Master of Philosophy in Physics & % iii Dedicated to all the sentient beings living in galaxies in the Virgo Cluster iv CONTENTS Synopsis : :::::::::::::::::::::::::::::::::::::: xvii Statement by Candidate :::::::::::::::::::::::::::::: xviii Acknowledgements ::::::::::::::::::::::::::::::::: xix 1. Introduction ::::::::::::::::::::::::::::::::::: 1 2. Low Surface Brightness (LSB) Galaxies :::::::::::::::::::: 5 2.1 Surface Brightness and LSB Galaxies De¯ned . 6 2.2 Physical Properties and Morphology . 8 2.3 Cluster and Field Distribution of LSB Dwarfs . 14 2.4 Galaxies, Cosmology and Clustering . 16 3. Galaxies and the Virgo Cluster :::::::::::::::::::::::: 19 3.1 Importance of the Virgo Cluster . 19 3.2 Galaxy Classi¯cation . 20 3.3 Virgo Galaxy Surveys and Catalogues . 24 3.4 Properties of the Virgo Cluster . 37 3.4.1 Velocity Distribution in the Direction of the Virgo Cluster . 37 3.4.2 Distance and 3D Structure . 38 vi Contents 3.4.3 Galaxy Population . 42 3.4.4 The Intra-Cluster Medium . 45 3.4.5 E®ects of the Cluster Environment . 47 4. Virgo Cluster Membership and the Luminosity Function :::::::::: 53 4.1 The Schechter Luminosity Function . 54 4.2 The Dwarf-to-Giant Ratio (DGR) . 58 4.3 Galaxy Detection . 59 4.4 Survey Completeness . 62 4.5 Virgo Cluster Membership . 63 4.5.1 Radial Velocities . 64 4.5.2 Morphology . 65 4.5.3 Concentration Parameters . 66 4.5.4 Scale Length Limits . 68 4.5.5 The Rines-Geller Threshold .
    [Show full text]
  • DGSAT: Dwarf Galaxy Survey with Amateur Telescopes
    Astronomy & Astrophysics manuscript no. arxiv30539 c ESO 2017 March 21, 2017 DGSAT: Dwarf Galaxy Survey with Amateur Telescopes II. A catalogue of isolated nearby edge-on disk galaxies and the discovery of new low surface brightness systems C. Henkel1;2, B. Javanmardi3, D. Mart´ınez-Delgado4, P. Kroupa5;6, and K. Teuwen7 1 Max-Planck-Institut f¨urRadioastronomie, Auf dem H¨ugel69, 53121 Bonn, Germany 2 Astronomy Department, Faculty of Science, King Abdulaziz University, P.O. Box 80203, Jeddah 21589, Saudi Arabia 3 Argelander Institut f¨urAstronomie, Universit¨atBonn, Auf dem H¨ugel71, 53121 Bonn, Germany 4 Astronomisches Rechen-Institut, Zentrum f¨urAstronomie, Universit¨atHeidelberg, M¨onchhofstr. 12{14, 69120 Heidelberg, Germany 5 Helmholtz Institut f¨ur Strahlen- und Kernphysik (HISKP), Universit¨at Bonn, Nussallee 14{16, D-53121 Bonn, Germany 6 Charles University, Faculty of Mathematics and Physics, Astronomical Institute, V Holeˇsoviˇck´ach 2, CZ-18000 Praha 8, Czech Republic 7 Remote Observatories Southern Alps, Verclause, France Received date ; accepted date ABSTRACT The connection between the bulge mass or bulge luminosity in disk galaxies and the number, spatial and phase space distribution of associated dwarf galaxies is a dis- criminator between cosmological simulations related to galaxy formation in cold dark matter and generalised gravity models. Here, a nearby sample of isolated Milky Way- class edge-on galaxies is introduced, to facilitate observational campaigns to detect the associated families of dwarf galaxies at low surface brightness. Three galaxy pairs with at least one of the targets being edge-on are also introduced. Approximately 60% of the arXiv:1703.05356v2 [astro-ph.GA] 19 Mar 2017 catalogued isolated galaxies contain bulges of different size, while the remaining objects appear to be bulgeless.
    [Show full text]