THE YOUNG ASTRONOMERS NEWSLETTER Volume 22 Number 12 STUDY + LEARN = POWER November 2014
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Studying the ISM at ∼ 10 Pc Scale in NGC 7793 with MUSE - I
Astronomy & Astrophysics manuscript no. dellabruna_2020 c ESO 2020 February 24, 2020 Studying the ISM at ∼ 10 pc scale in NGC 7793 with MUSE - I. Data description and properties of the ionised gas Lorenza Della Bruna1, Angela Adamo1, Arjan Bik1, Michele Fumagalli2; 3; 4, Rene Walterbos5, Göran Östlin1, Gustavo Bruzual6, Daniela Calzetti7, Stephane Charlot8, Kathryn Grasha9, Linda J. Smith10, David Thilker11, and Aida Wofford12 1 Department of Astronomy, Oskar Klein Centre, Stockholm University, AlbaNova University Centre, SE-106 91 Stockholm, Swe- den 2 Institute for Computational Cosmology, Durham University, South Road, Durham, DH1 3LE, UK 3 Centre for Extragalactic Astronomy, Durham University, South Road, Durham, DH1 3LE, UK 4 Dipartimento di Fisica G. Occhialini, Università degli Studi di Milano Bicocca, Piazza della Scienza 3, 20126 Milano, Italy 5 Department of Astronomy, New Mexico State University, Las Cruces, NM, 88001, USA 6 Instituto de Radioastronomía y Astrofísica, UNAM, Campus Morelia, Michoacan, C.P. 58089, México 7 Department of Astronomy, University of Massachusetts, Amherst, MA 01003, USA 8 Sorbonne Université, CNRS, UMR7095, Institut d’Astrophysique de Paris, F-75014, Paris, France 9 Research School of Astronomy and Astrophysics, Australian National University, Canberra, ACT 2611, Australia 10 Space Telescope Science Institute and European Space Agency, 3700 San Martin Drive, Baltimore, MD 2121, USA 11 Department of Physics and Astronomy, Johns Hopkins University, 3400 N. Charles Street, Baltimore, MD 21218, USA 12 Instituto de Astronomía, Universidad Nacional Autónoma de México, Unidad Académica en Ensenada, Km 103 Carr. Tijuana−Ensenada, Ensenada 22860, México Received XXX / Accepted YYY ABSTRACT Context. Studies of nearby galaxies reveal that around 50% of the total Hα luminosity in late-type spirals originates from diffuse ionised gas (DIG), which is a warm, diffuse component of the interstellar medium that can be associated with various mechanisms, the most important ones being ’leaking’ HII regions, evolved field stars, and shocks. -
Arxiv:Astro-Ph/0305472 V1 23 May 2003
Astronomy & Astrophysics manuscript no. (will be inserted by hand later) An Hα survey aiming at the detection of extraplanar diffuse ionized gas in halos of edge–on spiral galaxies ? II. The Hα survey atlas and catalog J. Rossa ??1,2 and R.–J. Dettmar1 1 Astronomisches Institut, Ruhr–Universit¨at Bochum, D–44780 Bochum, Germany e-mail: [email protected], [email protected] 2 Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, U.S.A. (present address) Received 14 February 2003 / Accepted 6 May 2003 Abstract. In this second paper on the investigation of extraplanar diffuse ionized gas in nearby edge–on spiral galaxies we present the actual results of the individual galaxies of our Hα imaging survey. A grand total of 74 galaxies have been studied, including the 9 galaxies of a recently studied sub–sample (Rossa & Dettmar 2000). 40.5% of all studied galaxies reveal extraplanar diffuse ionized gas, whereas in 59.5% of the survey galaxies no extraplanar diffuse ionized gas could be detected. The average distances of this extended emission above the galactic midplane range from 1–2 kpc, while individual filaments in a few galaxies reach distances of up to |z| ∼ 6 kpc. In several cases a pervasive layer of ionized gas was detected, similar to the Reynolds layer in our Milky Way, while other galaxies reveal only extended emission locally. The morphology of the diffuse ionized gas is discussed for each galaxy and is compared with observations of other important ISM constituents in the context of the disk–halo connection, in those cases where published results were available. -
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. -
Radiative Models for Jets in X-Ray Binaries
UNIVERSIDAD DE BUENOS AIRES Facultad de Ciencias Exactas y Naturales Departamento de Física Radiative models for jets in X-ray binaries A thesis submitted for the degree of Doctor of Philosophy in Physics Gabriela Soledad Vila Supervisor: Dr. Gustavo E. Romero Counsellor: Dr. Pablo D. Mininni Workplace: Instituto Argentino de Radioastronomía Buenos Aires, 2012 UNIVERSIDAD DE BUENOS AIRES Facultad de Ciencias Exactas y Naturales Departamento de Física Modelos radiativos para jets en binarias de rayos X Tesis presentada para optar al título de Doctor de la Universidad de Buenos Aires en el área Ciencias Físicas Gabriela Soledad Vila Director de Tesis: Dr. Gustavo E. Romero Consejero de Estudios: Dr. Pablo D. Mininni Lugar de Trabajo: Instituto Argentino de Radioastronomía Buenos Aires, 2012 This work has been awarded the Carlos M. Varsavsky Prize to the Best PhD Thesis on Astronomy and Astrophysics in Argentina 2010-2012, granted by the Astronomical Society of Argentina. Este trabajo ha sido galardonado con el Premio Carlos M. Varsavsky a la Mejor Tesis Doctoral en Astronomía y Astrofísica de la Argentina 2010-2012, otorgado por la Asociación Argentina de Astronomía. ABSTRACT Radiative models for jets in X-ray binaries An outstanding feature of astrophysical accreting sources at all scales in the Universe is the production of jets - collimated, bipolar, extended flows of matter and electromagnetic field ejected from the surroundings of a rotating object. Microquasars are X-ray binaries that produce relativistic jets. Jets in microquasars emit along the whole electromagnetic spectrum. The radiation is non-thermal; this reveals that jets accelerate particles up to relativistic energies. -
Jrasc-August'99 Text
Publications and Products of August/août 1999 Volume/volume 93 Number/numero 4 [678] The Royal Astronomical Society of Canada Observer’s Calendar — 2000 This calendar was created by members of the RASC. All photographs were taken by amateur astronomers using ordinary camera lenses and small telescopes and represent a wide spectrum of objects. An informative caption accompanies every photograph. This year all of the photos are in full colour. The Journal of the Royal Astronomical Society of Canada Le Journal de la Société royale d’astronomie du Canada It is designed with the observer in mind and contains comprehensive astronomical data such as daily Moon rise and set times, significant lunar and planetary conjunctions, eclipses, and meteor showers. The 1999 edition received two awards from the Ontario Printing and Imaging Association, Best Calendar and the Award of Excellence. (designed and produced by Rajiv Gupta). Price: $13.95 (members); $15.95 (non-members) (includes taxes, postage and handling) The Beginner’s Observing Guide This guide is for anyone with little or no experience in observing the night sky. Large, easy to read star maps are provided to acquaint the reader with the constellations and bright stars. Basic information on observing the moon, planets and eclipses through the year 2005 is provided. There is also a special section to help Scouts, Cubs, Guides and Brownies achieve their respective astronomy badges. Written by Leo Enright (160 pages of information in a soft-cover book with otabinding which allows the book to lie flat). Price: $15 (includes taxes, postage and handling) Looking Up: A History of the Royal Astronomical Society of Canada Published to commemorate the 125th anniversary of the first meeting of the Toronto Astronomical Club, “Looking Up — A History of the RASC” is an excellent overall history of Canada’s national astronomy organization. -
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. -
Key Information • This Exam Contains 6 Parts, 79 Questions, and 180 Points Total
Reach for the Stars *** Practice Test 2020-2021 Season Answer Key Information • This exam contains 6 parts, 79 questions, and 180 points total. • You may take this test apart. Put your team number on each page. There is not a separate answer page, so write all answers on this exam. • You are permitted the resources specified on the 2021 rules. • Don't worry about significant figures, use 3 or more in your answers. However, be sure your answer is in the correct units. • For calculation questions, any answers within 10% (inclusive) of the answer on the key will be accepted. • Ties will be broken by section score in reverse order (i.e. Section F score is the first tiebreaker, Section A the last). • Written by RiverWalker88. Feel free to PM me if you have any questions, feedback, etc. • Good Luck! Reach for the stars! Reach for the Stars B Team #: Constants and Conversions CONSTANTS Stefan-Boltzmann Constant = σ = 5:67 × 10−8 W=m2K4 Speed of light = c = 3 × 108m/s 30 Mass of the sun = M = 1:99 × 10 kg 5 Radius of the sun = R = 6:96 × 10 km Temperature of the sun = T = 5778K 26 Luminosity of the sun = L = 3:9 × 10 W Absolute Magnitude of the sun = MV = 4.83 UNIT CONVERSIONS 1 AU = 1:5 × 106km 1 ly = 9:46 × 1012km 1 pc = 3:09 × 1013km = 3.26 ly 1 year = 31557600 seconds USEFUL EQUATIONS 2900000 Wien's Law: λ = peak T • T = Temperature (K) • λpeak = Peak Wavelength in Blackbody Spectrum (nanometers) 1 Parallax: d = p • d = Distance (pc) • p = Parallax Angle (arcseconds) Page 2 of 13Page 13 Reach for the Stars B Team #: Part A: Astrophotographical References 9 questions, 18 points total For each of the following, identify the star or deep space object pictured in the image. -
An H-Alpha Survey Aiming at the Detection of Extraplanar Diffuse
Astronomy & Astrophysics manuscript no. (will be inserted by hand later) An Hα survey aiming at the detection of extraplanar diffuse ionized gas in halos of edge–on spiral galaxies ⋆ II. The Hα survey atlas and catalog J. Rossa ⋆⋆1,2 and R.–J. Dettmar1 1 Astronomisches Institut, Ruhr–Universit¨at Bochum, D–44780 Bochum, Germany e-mail: [email protected], [email protected] 2 Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, U.S.A. (present address) Received 14 February 2003 / Accepted 6 May 2003 Abstract. In this second paper on the investigation of extraplanar diffuse ionized gas in nearby edge–on spiral galaxies we present the actual results of the individual galaxies of our Hα imaging survey. A grand total of 74 galaxies have been studied, including the 9 galaxies of a recently studied sub–sample (Rossa & Dettmar 2000). 40.5% of all studied galaxies reveal extraplanar diffuse ionized gas, whereas in 59.5% of the survey galaxies no extraplanar diffuse ionized gas could be detected. The average distances of this extended emission above the galactic midplane range from 1–2 kpc, while individual filaments in a few galaxies reach distances of up to |z| ∼ 6 kpc. In several cases a pervasive layer of ionized gas was detected, similar to the Reynolds layer in our Milky Way, while other galaxies reveal only extended emission locally. The morphology of the diffuse ionized gas is discussed for each galaxy and is compared with observations of other important ISM constituents in the context of the disk–halo connection, in those cases where published results were available. -
MY SO October Showdown Rules
S P A C E - O C T O B E R 2 0 2 0 MY SO STEM SHOWDOWN C O N T E N T , R E C O M M E N D E D M A T E R I A L S & S C O R I N G STEM SHOWDOWN CONTENT The STEM Showdown will consist of a series of online multiple-choice questions. Middle school (Grade 6-9) participant questions will center around the properties and evolution of stars and galaxies as well as their observation using different portions of the electromagnetic spectrum (e.g., Radio, Infrared, Visible, Ultraviolet, X-Ray, Gamma Ray). While high school (Grades 9-12) participants will focus on Star and Galaxy Formation and Evolution. A Showdown participant will have 55- minutes to answer as many questions as possible. The middle school (Grades 6-9) content and skills covered by the Showdown this month is as follows: 1.Stellar and galactic evolution 2.Spectral classification of stars 3.Hubble classification of galaxies 4.Observation using multiple portions of the electromagnetic spectrum 5.The relationship between stellar temperature, radius, and luminosity 6.Magnitude and luminosity scales, distance modulus, inverse square law 7.Identification of the stars, constellations, and deep sky objects included in the list below as they appear on star charts, H-R diagrams, portable star labs, photos, or planetariums. Note: Constellations are underlined; Stars are boldface; Deep Sky Objects are italicized. a.Andromeda: M31 (Andromeda Galaxy) b.Aquila: Altair c.Auriga: Capella d.Bootes: Arcturus e.Cancer: DLA0817g f.Canis Major: Sirius g.Canis Minor: Procyon h.Centaurus: NGC5128 i.Coma Berenices: NGC4676, NGC4555 j.Corvus: NGC4038/NGC4039 k.Crux: Dragonfish Nebula l.Cygnus: Deneb m.Dorado: 30 Doradus, LMC n.Gemini: Castor, Pollux o.Lyra: Vega p.Ophiuchus: Zeta Ophiuchi, Rho Ophiuchi cloud complex q.Orion: Betelgeuse, Rigel & M42 (Orion Nebula) r.Perseus: Algol, NGC1333 Science Olympiad, Inc. -
Prime Focus (10-08)
Highlights of the October Sky. -- -- -- 1st -- -- -- Dusk: Thin crescent Moon visible low in WSW. Look PPrime Focuss 5º or 6º below Venus. A Publication of the Kalamazoo Astronomical Society -- -- -- 6th -- -- -- PM: Moon lower right of Jupiter. October 2008 -- -- -- 7th -- -- -- PM: Moon lower left of Jupiter. ThisThis MonthsMonths KAS EventsEvents -- -- -- 7th -- -- -- First Quarter Moon -- -- -- 14th -- -- -- General Meeting: Friday, October 3 @ 7:00 pm Full Moon Kalamazoo Math & Science Center - See Page 12 for Details -- -- -- 17th -- -- -- Dawn: Mercury visible 5º Observing Session: Saturday, October 4 @ 7:00 pm above the eastern horizon until the 30th. Overwhelming Open Clusters - Kalamazoo Nature Center st -- -- -- 21st -- -- -- Board Meeting: Sunday, October 5 @ 5:00 pm Last Quarter Moon Sunnyside Church - 2800 Gull Road - All Members Welcome AM: Orionid Meteor AM: Orionid Meteor Shower (10 -- 2020 meteorsmeteors per hour). Observing Session: Saturday, October 25 @ 7:00 pm The Great Square - Kalamazoo Nature Center -- -- -- 23rd -- -- -- Dawn: Waning Crescent Moon upper right of Alpha Leonis (Regulus). -- -- -- 24th -- -- -- Dawn: Waning Crescent InsideInside thethe Newsletter.Newsletter. .. .. Moon between Saturn and Regulus. September Meeting Minutes................ p. 2 -- -- -- 25th -- -- -- Board Meeting Minutes......................... p. 3 Dawn: Moon below Saturn Intelligent Imaging................................... p. 4 -- -- -- 25th -- -- -- Dusk: Venus is passing Astronomy Software............................ -
190 Index of Names
Index of names Ancora Leonis 389 NGC 3664, Arp 005 Andriscus Centauri 879 IC 3290 Anemodes Ceti 85 NGC 0864 Name CMG Identification Angelica Canum Venaticorum 659 NGC 5377 Accola Leonis 367 NGC 3489 Angulatus Ursae Majoris 247 NGC 2654 Acer Leonis 411 NGC 3832 Angulosus Virginis 450 NGC 4123, Mrk 1466 Acritobrachius Camelopardalis 833 IC 0356, Arp 213 Angusticlavia Ceti 102 NGC 1032 Actenista Apodis 891 IC 4633 Anomalus Piscis 804 NGC 7603, Arp 092, Mrk 0530 Actuosus Arietis 95 NGC 0972 Ansatus Antliae 303 NGC 3084 Aculeatus Canum Venaticorum 460 NGC 4183 Antarctica Mensae 865 IC 2051 Aculeus Piscium 9 NGC 0100 Antenna Australis Corvi 437 NGC 4039, Caldwell 61, Antennae, Arp 244 Acutifolium Canum Venaticorum 650 NGC 5297 Antenna Borealis Corvi 436 NGC 4038, Caldwell 60, Antennae, Arp 244 Adelus Ursae Majoris 668 NGC 5473 Anthemodes Cassiopeiae 34 NGC 0278 Adversus Comae Berenices 484 NGC 4298 Anticampe Centauri 550 NGC 4622 Aeluropus Lyncis 231 NGC 2445, Arp 143 Antirrhopus Virginis 532 NGC 4550 Aeola Canum Venaticorum 469 NGC 4220 Anulifera Carinae 226 NGC 2381 Aequanimus Draconis 705 NGC 5905 Anulus Grahamianus Volantis 955 ESO 034-IG011, AM0644-741, Graham's Ring Aequilibrata Eridani 122 NGC 1172 Aphenges Virginis 654 NGC 5334, IC 4338 Affinis Canum Venaticorum 449 NGC 4111 Apostrophus Fornac 159 NGC 1406 Agiton Aquarii 812 NGC 7721 Aquilops Gruis 911 IC 5267 Aglaea Comae Berenices 489 NGC 4314 Araneosus Camelopardalis 223 NGC 2336 Agrius Virginis 975 MCG -01-30-033, Arp 248, Wild's Triplet Aratrum Leonis 323 NGC 3239, Arp 263 Ahenea -
Exótico Cielo Profundo 9
9 El escultor de galaxias Sculptor (Scl) Sculptoris. Escultor. · Exótico Cielo Profundo 9 de Rodolfo Ferraiuolo y Enzo De Bernardini Constelación Sculptor (Scl) Época Comienzos de la Primavera Austral Blanco 1 NGC 55 NGC 131 NGC 134 NGC 150 HD 4113 HD 4208 Objetos NGC 253 NGC 289 NGC 288 NGC 300 SDEG NGC 7793 El comienzo de la primavera austral es una gran ocasión para explorar algunos magníficos objetos de Sculptor, constelación creada en el año 1752 por el astrónomo rumano-francés Nicolai-Ludovici De La Caille, más conocido como Nicolás-Louis de Lacaille. Dentro de sus límites encontramos a, la mayoría de una veintena de galaxias, del tipo tardío, de un cercano (el más próximo al Grupo Local) y pequeño grupo, bautizado en 1959 por el astrónomo francés G. de Vaucouleurs como Grupo de Sculptor y, en 1960 por el astrónomo argentino J. L. Sérsic, Grupo del Polo Sur Galáctico, debido a que sus miembros se localizan agrupados en dirección al Polo Sur Galáctico. De este sugestivo grupo elegimos algunas hermosas galaxias que, estudiaremos junto a otros interesantes objetos más, como el cúmulo globular NGC 288, el cúmulo abierto Blanco 1, otras galaxias lejanas y, como curiosidad ya que no es habitual en la sección, veremos un par de brillantes estrellas con exoplanetas. Nuestro punto de partida será al Sur de la constelación, donde estudiaremos a NGC 300. Esta bonita galaxia espiral, clase SA(s)d, es miembro del Grupo del Polo Galáctico Sur y, fue descubierta por J. Dunlop en el año 1826, unos 8 años antes que J.