NCRAL Northern Lights Winter 2021
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
THE STAR FORMATION NEWSLETTER an Electronic Publication Dedicated to Early Stellar Evolution and Molecular Clouds
THE STAR FORMATION NEWSLETTER An electronic publication dedicated to early stellar evolution and molecular clouds No. 90 — 27 March 2000 Editor: Bo Reipurth ([email protected]) Abstracts of recently accepted papers The Formation and Fragmentation of Primordial Molecular Clouds Tom Abel1, Greg L. Bryan2 and Michael L. Norman3,4 1 Harvard Smithsonian Center for Astrophysics, MA, 02138 Cambridge, USA 2 Massachusetts Institute of Technology, MA, 02139 Cambridge, USA 3 LCA, NCSA, University of Illinois, 61801 Urbana/Champaign, USA 4 Astronomy Department, University of Illinois, Urbana/Champaign, USA E-mail contact: [email protected] Many questions in physical cosmology regarding the thermal history of the intergalactic medium, chemical enrichment, reionization, etc. are thought to be intimately related to the nature and evolution of pregalactic structure. In particular the efficiency of primordial star formation and the primordial IMF are of special interest. We present results from high resolution three–dimensional adaptive mesh refinement simulations that follow the collapse of primordial molecular clouds and their subsequent fragmentation within a cosmologically representative volume. Comoving scales from 128 kpc down to 1 pc are followed accurately. Dark matter dynamics, hydrodynamics and all relevant chemical and radiative processes (cooling) are followed self-consistently for a cluster normalized CDM structure formation model. Primordial molecular clouds with ∼ 105 solar masses are assembled by mergers of multiple objects that have formed −4 hydrogen molecules in the gas phase with a fractional abundance of ∼< 10 . As the subclumps merge cooling lowers the temperature to ∼ 200 K in a “cold pocket” at the center of the halo. Within this cold pocket, a quasi–hydrostatically > 5 −3 contracting core with mass ∼ 200M and number densities ∼ 10 cm is found. -
C a L E N D a R F O R 2019
Small Astronomy Calendar for Amateur Astronomers Year III 2021 Let’s welcome our 2021 Small Astronomy Calendar Edition made by our Intergalactic Astronomy Educators Fellowship (IGAEF)’s team. In 2021, many amateur astronomers asked for calculations for more specific geographical locations. This year we added new useful calculated positions and coordinates for everyone in the world to use. You should check this calendar every month, specifically the lunar occultations pages for your observation point. There are many interesting and unique events that might not happen every year, because of the different parameters of the Moon orbit. Our hope is to fulfill your expectations. We would like to receive suggestions and feedback. You can find the editor’s email in the last page of the calendar. We appreciate your support and we are looking forward to having a good observational year, and a better and more complete calendar for this first year of a new decade. Index 3 - Calendar for 2021 4 – What is the Intergalactic Astronomy Educators Fellowship (IGAEF) 5 - Time Zones and Universal Time 6 - Phases of the Moon 2021 7 – Physical Ephemeris for the Moon 2021 10 - Local Time (EST) of MOONRISE 2021 11 - Local Time (EST) of MOONSET 2021 12 - Local time (EST) of planets rise and set 2021 15 - Diary of Astronomical Phenomena 2021 21 - Lunar eclipses 23 - Solar Eclipses 25 - Meteor Showers for 2021 26 – 2021 UPCOMING COMETS 27 - Satellites of Jupiter 2021 36 – Mutual Events of Jupiter Satellites 2021 39 - Julian Day Number, Apparent Sidereal Time, Obliquity -
A PRIMEIRA REVISTA ELETRÔNICA BRASILEIRA EXCLUSIVA DE ASTRONOMIA Revista Macrocosm O.Com Ano II - Edição N° 14 - Janeiro De 2005
A PRIMEIRA REVISTA ELETRÔNICA BRASILEIRA EXCLUSIVA DE ASTRONOMIA revista macroCOSM O.com Ano II - Edição n° 14 - Janeiro de 2005 Editorial Redação [email protected] Desde tempos imemoriáveis o homem tem olhado Diretor Editor Chefe para o céu. No início, a observação do movimento Hemerson Brandão [email protected] gradual dos corpos celestes ajudou aos primórdios da civilização na contagem e regularização do tempo, e por esse motivo, a Astronomia é considerada uma das Diagramadores Rodolfo Saccani ciências mais antigas da humanidade. [email protected] Foi na Antiga Grécia, por volta de 450 a.C., que os Sharon Camargo gregos começaram a fazer os primeiros registros [email protected] detalhados do movimento dos astros, tentando entender Hemerson Brandão [email protected] as suas causas. Ricas histórias mitológicas explicavam o porque de cada constelação no céu, enquanto filósofos debatiam uma explicação para o movimento Redatores Audemário Prazeres dos astros errantes, os planetas. [email protected] Atualmente parte desse conhecimento foi Hélio “Gandhi” Ferrari sobrepujado por anos de conhecimentos científicos [email protected] adquiridos ao longo da história, mas muitos resquícios Laércio F. Oliveira [email protected] ainda são encontrados na Astronomia Moderna. Os Marco Valois primeiros estudos do movimento da Terra, como por [email protected] exemplo a precessão dos equinócios, o desenho da Naelton M. Araujo maioria das constelações, a escala de magnitudes [email protected] Paulo R. Monteiro estelares e até mesmo os primeiros catálogos de [email protected] estrelas, são a herança da rica cultura grega. Sem Rosely Grégio dúvida, a base para todo o pensamento científico atual. -
Winter Observing Notes
Wynyard Planetarium & Observatory Winter Observing Notes Wynyard Planetarium & Observatory PUBLIC OBSERVING – Winter Tour of the Sky with the Naked Eye NGC 457 CASSIOPEIA eta Cas Look for Notice how the constellations 5 the ‘W’ swing around Polaris during shape the night Is Dubhe yellowish compared 2 Polaris to Merak? Dubhe 3 Merak URSA MINOR Kochab 1 Is Kochab orange Pherkad compared to Polaris? THE PLOUGH 4 Mizar Alcor Figure 1: Sketch of the northern sky in winter. North 1. On leaving the planetarium, turn around and look northwards over the roof of the building. To your right is a group of stars like the outline of a saucepan standing up on it’s handle. This is the Plough (also called the Big Dipper) and is part of the constellation Ursa Major, the Great Bear. The top two stars are called the Pointers. Check with binoculars. Not all stars are white. The colour shows that Dubhe is cooler than Merak in the same way that red-hot is cooler than white-hot. 2. Use the Pointers to guide you to the left, to the next bright star. This is Polaris, the Pole (or North) Star. Note that it is not the brightest star in the sky, a common misconception. Below and to the right are two prominent but fainter stars. These are Kochab and Pherkad, the Guardians of the Pole. Look carefully and you will notice that Kochab is slightly orange when compared to Polaris. Check with binoculars. © Rob Peeling, CaDAS, 2007 version 2.0 Wynyard Planetarium & Observatory PUBLIC OBSERVING – Winter Polaris, Kochab and Pherkad mark the constellation Ursa Minor, the Little Bear. -
Binocular Double Star Logbook
Astronomical League Binocular Double Star Club Logbook 1 Table of Contents Alpha Cassiopeiae 3 14 Canis Minoris Sh 251 (Oph) Psi 1 Piscium* F Hydrae Psi 1 & 2 Draconis* 37 Ceti Iota Cancri* 10 Σ2273 (Dra) Phi Cassiopeiae 27 Hydrae 40 & 41 Draconis* 93 (Rho) & 94 Piscium Tau 1 Hydrae 67 Ophiuchi 17 Chi Ceti 35 & 36 (Zeta) Leonis 39 Draconis 56 Andromedae 4 42 Leonis Minoris Epsilon 1 & 2 Lyrae* (U) 14 Arietis Σ1474 (Hya) Zeta 1 & 2 Lyrae* 59 Andromedae Alpha Ursae Majoris 11 Beta Lyrae* 15 Trianguli Delta Leonis Delta 1 & 2 Lyrae 33 Arietis 83 Leonis Theta Serpentis* 18 19 Tauri Tau Leonis 15 Aquilae 21 & 22 Tauri 5 93 Leonis OΣΣ178 (Aql) Eta Tauri 65 Ursae Majoris 28 Aquilae Phi Tauri 67 Ursae Majoris 12 6 (Alpha) & 8 Vul 62 Tauri 12 Comae Berenices Beta Cygni* Kappa 1 & 2 Tauri 17 Comae Berenices Epsilon Sagittae 19 Theta 1 & 2 Tauri 5 (Kappa) & 6 Draconis 54 Sagittarii 57 Persei 6 32 Camelopardalis* 16 Cygni 88 Tauri Σ1740 (Vir) 57 Aquilae Sigma 1 & 2 Tauri 79 (Zeta) & 80 Ursae Maj* 13 15 Sagittae Tau Tauri 70 Virginis Theta Sagittae 62 Eridani Iota Bootis* O1 (30 & 31) Cyg* 20 Beta Camelopardalis Σ1850 (Boo) 29 Cygni 11 & 12 Camelopardalis 7 Alpha Librae* Alpha 1 & 2 Capricorni* Delta Orionis* Delta Bootis* Beta 1 & 2 Capricorni* 42 & 45 Orionis Mu 1 & 2 Bootis* 14 75 Draconis Theta 2 Orionis* Omega 1 & 2 Scorpii Rho Capricorni Gamma Leporis* Kappa Herculis Omicron Capricorni 21 35 Camelopardalis ?? Nu Scorpii S 752 (Delphinus) 5 Lyncis 8 Nu 1 & 2 Coronae Borealis 48 Cygni Nu Geminorum Rho Ophiuchi 61 Cygni* 20 Geminorum 16 & 17 Draconis* 15 5 (Gamma) & 6 Equulei Zeta Geminorum 36 & 37 Herculis 79 Cygni h 3945 (CMa) Mu 1 & 2 Scorpii Mu Cygni 22 19 Lyncis* Zeta 1 & 2 Scorpii Epsilon Pegasi* Eta Canis Majoris 9 Σ133 (Her) Pi 1 & 2 Pegasi Δ 47 (CMa) 36 Ophiuchi* 33 Pegasi 64 & 65 Geminorum Nu 1 & 2 Draconis* 16 35 Pegasi Knt 4 (Pup) 53 Ophiuchi Delta Cephei* (U) The 28 stars with asterisks are also required for the regular AL Double Star Club. -
Ov\,E <1000{ Tayget
oV\,e <1000{ TaYget w~tVi SOVlA.e otViey s~gVits wortVt see~v\'g wVi~Le You'ye ~v\, tVie Ne~gVtboYVioofi MlAycltl GLustey M4g wLtVi ~cn'bov\" stClr X CClv\"~rL Cl V\.,c{ Cl v\"L~e grou-p of stClYS Cl rouV\.,c{ "B>etCl CCl V\.,Ls M~v\"orLs Cluster M48, a magnitude 5.5 open star cluster in the constellation Hydra, was first discovered by comet-hunter Charles Messier in 1771 but, because Messier misstated its coordinates, it was "lost" until 1934, when German astronomer Oswalt Thomas demonstrated that the cluster Messier described was NGC 2458. The cluster is shown slightly right of center near the bottom of the chart, along with other nearby stars that we will use in this month's hunt: • Pollux • • • • • • Gamma M44 • Cancer. • • ~ • ;. I • ·HYdra~ Procyon •• • Sextans • • Monoceros • 0 ~\ • M48 . To find M48 using binoculars or a finderscope, start at Procyon, the bright mag 0.3 star at the SE corner of The Winter Hexagon. Procyon is the 8th brightest star in the sky, and quite close to us, at a distance of only 11~ light years. It was named Procyon, meaning "Before the Dog," because it rises just before Sirius, The Dog Star: that was important because Sirius heralded the annual flooding of the Nile River, which was crucial to the life of ancient Egypt. Just over 4° NW of Procyon is mag 2.9 blue dwarf Beta Canis Minoris, which forms a pretty lYz ° binocular group with a mag 4.3 orange giant and a mag 5.0 yellow giant. -
Downloads/ Astero2007.Pdf) and by Aerts Et Al (2010)
This work is protected by copyright and other intellectual property rights and duplication or sale of all or part is not permitted, except that material may be duplicated by you for research, private study, criticism/review or educational purposes. Electronic or print copies are for your own personal, non- commercial use and shall not be passed to any other individual. No quotation may be published without proper acknowledgement. For any other use, or to quote extensively from the work, permission must be obtained from the copyright holder/s. i Fundamental Properties of Solar-Type Eclipsing Binary Stars, and Kinematic Biases of Exoplanet Host Stars Richard J. Hutcheon Submitted in accordance with the requirements for the degree of Doctor of Philosophy. Research Institute: School of Environmental and Physical Sciences and Applied Mathematics. University of Keele June 2015 ii iii Abstract This thesis is in three parts: 1) a kinematical study of exoplanet host stars, 2) a study of the detached eclipsing binary V1094 Tau and 3) and observations of other eclipsing binaries. Part I investigates kinematical biases between two methods of detecting exoplanets; the ground based transit and radial velocity methods. Distances of the host stars from each method lie in almost non-overlapping groups. Samples of host stars from each group are selected. They are compared by means of matching comparison samples of stars not known to have exoplanets. The detection methods are found to introduce a negligible bias into the metallicities of the host stars but the ground based transit method introduces a median age bias of about -2 Gyr. -
FY13 High-Level Deliverables
National Optical Astronomy Observatory Fiscal Year Annual Report for FY 2013 (1 October 2012 – 30 September 2013) Submitted to the National Science Foundation Pursuant to Cooperative Support Agreement No. AST-0950945 13 December 2013 Revised 18 September 2014 Contents NOAO MISSION PROFILE .................................................................................................... 1 1 EXECUTIVE SUMMARY ................................................................................................ 2 2 NOAO ACCOMPLISHMENTS ....................................................................................... 4 2.1 Achievements ..................................................................................................... 4 2.2 Status of Vision and Goals ................................................................................. 5 2.2.1 Status of FY13 High-Level Deliverables ............................................ 5 2.2.2 FY13 Planned vs. Actual Spending and Revenues .............................. 8 2.3 Challenges and Their Impacts ............................................................................ 9 3 SCIENTIFIC ACTIVITIES AND FINDINGS .............................................................. 11 3.1 Cerro Tololo Inter-American Observatory ....................................................... 11 3.2 Kitt Peak National Observatory ....................................................................... 14 3.3 Gemini Observatory ........................................................................................ -
THE STAR FORMATION NEWSLETTER an Electronic Publication Dedicated to Early Stellar Evolution and Molecular Clouds
THE STAR FORMATION NEWSLETTER An electronic publication dedicated to early stellar evolution and molecular clouds No. 193 — 13 Jan 2009 Editor: Bo Reipurth ([email protected]) Abstracts of recently accepted papers [O i] sub-arcsecond study of a microjet from an intermediate mass young star: RY Tau V. Agra-Amboage1, C. Dougados1, S. Cabrit2, P.J.V. Garcia3,4,1 and P. Ferruit5 1 Laboratoire d’Astrophysique de l’Observatoire de Grenoble, UMR 5521 du CNRS, 38041 Grenoble C´edex 9, France 2 LERMA, Observatoire de Paris, UMR 8112 du CNRS, 61 Avenue de l’Observatoire, 75014 Paris, France 3 Departamento de Engenharia Fisica,Faculdade de Engenharia,Universidade do Porto, 4200-465 Porto, Portugal 4 Centro de Astrofisica, Universidade do Porto, Porto, Portugal 5 CRAL, Observatoire de Lyon, 9 Av. Charles Andr´e, F-69230 St. Genis Laval, France E-mail contact: Catherine.Dougados at obs.ujf-grenoble.fr High-resolution studies of microjets in T Tauri stars (cTTs) reveal key information on the jet collimation and launching mechanism, but only a handful of systems have been mapped so far. We perform a detailed study of the microjet from the 2 M⊙ young star RY Tau, to investigate the influence of its higher stellar mass and claimed close binarity on jet properties. Spectro-imaging observations of RY Tau were obtained in [O i]λ6300 with resolutions of 0.4′′ and 135 km s−1, using the integral field spectrograph OASIS at the Canada-France-Hawaii Telescope. Deconvolved images reach a resolution of 0.2′′. The blueshifted jet is detected within 2′′ of the central star. -
GEORGE HERBIG and Early Stellar Evolution
GEORGE HERBIG and Early Stellar Evolution Bo Reipurth Institute for Astronomy Special Publications No. 1 George Herbig in 1960 —————————————————————– GEORGE HERBIG and Early Stellar Evolution —————————————————————– Bo Reipurth Institute for Astronomy University of Hawaii at Manoa 640 North Aohoku Place Hilo, HI 96720 USA . Dedicated to Hannelore Herbig c 2016 by Bo Reipurth Version 1.0 – April 19, 2016 Cover Image: The HH 24 complex in the Lynds 1630 cloud in Orion was discov- ered by Herbig and Kuhi in 1963. This near-infrared HST image shows several collimated Herbig-Haro jets emanating from an embedded multiple system of T Tauri stars. Courtesy Space Telescope Science Institute. This book can be referenced as follows: Reipurth, B. 2016, http://ifa.hawaii.edu/SP1 i FOREWORD I first learned about George Herbig’s work when I was a teenager. I grew up in Denmark in the 1950s, a time when Europe was healing the wounds after the ravages of the Second World War. Already at the age of 7 I had fallen in love with astronomy, but information was very hard to come by in those days, so I scraped together what I could, mainly relying on the local library. At some point I was introduced to the magazine Sky and Telescope, and soon invested my pocket money in a subscription. Every month I would sit at our dining room table with a dictionary and work my way through the latest issue. In one issue I read about Herbig-Haro objects, and I was completely mesmerized that these objects could be signposts of the formation of stars, and I dreamt about some day being able to contribute to this field of study. -
Journal of the Association of Lunar & Planetary Observers
ISSN-0039-2502 Journal of the Association of Lunar & Planetary Observers The Strolling Astronomer Volume 54, Number 1, Winter 2012 Now in Portable Document Format (PDF) for Macintosh and PC-compatible computers Online and in COLOR at http://www.alpo-astronomy.org Inside this issue . • ALCon 2012 information • What’s REALLY up with those Venusian clouds? • Whole-disk brightness measurements of Mars • A ‘Great White Spot’ on Saturn? • The Remote Planets in 2010 and 2011 . plus reports about your ALPO section activities and much, much more! Online image of the December 11, 2011 lunar eclipse taken by “Shutter Shooter” on the Gold Coast, Queensland, Australia. The first moon was taken at 10:30 pm local time, the second moon at 11:20 pm, the third moon 12:00midnight and the last blood-red moon was taken at 1:15 a.m. According to his web page, a Pentax X90 12.1 megapixel digital camera was used for image-capture, and Adobe PhotoShop CS5 was used to stitch the photos together and added a small amount of contrast/ brightness. Source: http://shutter-shooter.deviantart.com/art/Lunar-Eclipse-December-2011-273379748 Your Affordable Since 1975 Astro-Imaging Source #9534 ED80T Carbon Fiber Triplet Apochromatic Refractor $799.99 #9534 ED102T Carbon Fiber Triplet Apochromatic Refractor $1,999.99 #9530 The Leo Trio (M65, M66 and NGC 3628) – Taken with the Orion ED102T CF Refractor, StarShoot Pro V2.0, Orion Atlas EQ-G, and Orion StarShoot AutoGuider. 23 x 10 minute #9530 exposures combined. Orion image. StarShoot™ G3 Deep Space StarShoot™ AllSky Magnificent Mini AutoGuider Package Imaging Camera Camera $349.99 #24781 $499.99 #53082 Color $899.99 $499.99 #53083 Mono #52187 NTSC Std. -
February 2000 the Albuquerque Astronomical Society News Letter
Back to List of Newsletters February 2000 This special HTML version of our newsletter contains most of the information published in the "real" Sidereal Times . All information is copyrighted by TAAS. Permission for other amateur astronomy associations is granted provided proper credit is given. Table of Contents Departments Calendars Lead Story: Ode to Spring: The Messier Marathon Presidents Update The Board Meeting Observatory Committee No report this month Last Month's General Meeting Recap Next General Meeting Observer's Page What's Up for February No report this month Ask the Experts: The Kids' Corner ATM Corner: Star Myths and More UNM Campus Observatory Report Docent News Astronomy 101 Astronomical Computing No report this month Internet Info GNTO News Trivia Question No trivia this month Letters to the Editor Lost and Found No items this month Classified Ads Feature Stories New CCD camera (and class) Project Astro New Mexico State Parks Rio Grande Nature Center Star Party TAAS Astronomy Day Call to Battle Library News Science Fair Judges Needed Astronomy Speaker Needed Misc Stuff Please note: TAAS offers a Safety Escort Service to those attending monthly meetings on the UNM campus. Please contact the President or any board member during social hour after the meeting if you wish assistance, and a Society member will happily accompany you to your car. Calendars Calendar Images March 2000 Calendar o GIF version (~65K) o PDF version (~20K) April 2000 Calendar o GIF version (~65K) o PDF version (~20K) TAAS Calendar page Ode to Spring: The Messier Marathon by Dave Brown Ah the approach of Spring, who can resist its overwhelming appeal.