Program Schedule: Proud of This Still Working Observatory Along with the Programs Are at 7:30 at Exhibits
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
Gamma Leonis B
Gamma Leonis b The planetary system Gamma Leonis hosts at least one planet. Note that the system is a multiple star system. It hosts at least 2 stellar components. System parameters. Primary system name. Gamma Leonis. Alternative system names. N/A. Gamma-2 Leonis. Alternative star names. gamma 1 Leo, gam01 Leo, γ1 Leo, γ1 Leonis, γ Leo A, Gamma Leonis A, gamma Leo A, gam Leo A, Algieba A, Al Gieba A, HD 89484, HIP 50583 A, TYC 1423-1349-1, SAO 81298, BD+20 2467 A, WDS J10200+1950 A, STF 1424 A. Gamma Leonis's wiki: Gamma Leonis (γ Leo, γ Leonis) is a binary star system in the constellation Leo. It has the traditional name Algieba or Al Gieba . Name origin and history The name Algieba originates from the Arabic الجبهة Al-Jabhah Gamma Leonis b is an extrasolar planet located 125.5 light years away in the constellation Leo, orbiting the giant star Gamma Leonis. On November 6, 2009, a planetary companion around primary star Gamma1 Leonis has been announced. Moreover radial velocity variations would also hint two strong signals at 8.5 and 1340 days. The former periodicity is likely due to stellar pulsation, whereas the latter could be indicative of the presence of an additional planetary companion with 2.14 Jupiter masses Gamma Leonis (γ Leo / γ Leonis) is a binary star system in the constellation Leo. It also has the traditional name Algieba or Al Gieba. Name origin and history. The name "Algieba" originates from the Arabic "Al-Jabhah", meaning "the forehead". -
Exo-Mercat a Merged Exoplanet Catalog
Exo-MerCat a merged exoplanet catalog 1,2 Eleonora Alei , Riccardo Claudi1, Andrea Bignamini3, Marco Molinaro3 1 INAF – Osservatorio Astronomico di Padova 2 DFA-UNIPD – Dipartimento di Fisica e Astronomia dell’Università degli Studi di Padova 3 INAF – Osservatorio Astronomico di Trieste IVOA Interoperability meeting Paris, 12-17 May 2019 Overview • Online exoplanet catalogs: state of the art • Raw statistics with the current datasets • Known Issues: updates, errors, selection criteria • Exo-MerCat: aims, description, efficiency • Update workflow and VO resource NASA Exoplanet Archive (NASA) Exoplanets Orbit Database (ORG) Open Exoplanet Catalogue (OEC) Extrasolar Planets Encyclopaedia (EU) Yikes! Raw statistics Raw Problems Selection Criteria Aliases Coordinates Updates - Names appear in different - Human errors (plus-minus - False positives are present in formats; signs); the catalogs because of lags - Whitespaces are present; - Not updated coordinates; in the updates; - Different aliases for the same - Different epochs. - New candidates have yet to be planet; included in the database. Algieba, gamma Leonis: Proxima Centauri b (ra,dec): in NASA: gam 1 Leo in NASA: (217.428995,-62.679485) in ORG: gamma Leo A in ORG: (217.448946,-62.681353) in EU: gamma 1 Leo in EU: (217.429167,-62.679444) in OEC: Gamma Leonis in OEC: (219.990850,-60.835619) 5 Aims • Provide greater uniformity among the databases; • More effective associations among the datasets; • Identify and correct errors, to warn the catalog maintainers; Exo-MerCat • Provide a direct link with most stellar sources archives; • Provide the user with an intuitive Graphical Interface to download and filter data. 6 Icons made by https://www.flaticon.com/authors/gregor-cresnar from www.flaticon.com Description Initialization • Create a nested folder to contain all useful files; • Use various Virtual Observatory tools to download raw datasets: Exo-MerCat • wget command to access NASA/ORG database; • git commands and an *.xml reader to access the OEC database; • VO TAP service for the EU database. -
Vssc163 Draftv3 IBVS 2 Colour Correct Graph.Pmd
British Astronomical Association VARIABLE STAR SECTION CIRCULAR No 163, March 2015 Contents IBVS 6080 – 6109 - J. Simpson ............................................... inside front cover From the Director - R. Pickard ........................................................................... 3 Polar V1432 Aquilae - Editor’s Note .................................................................. 4 Eclipsing Binary News - D. Loughney .............................................................. 4 Update on the Campaign to Observe the Dwarf Nova CSS 121005:212625+201948 - J. Shears ............... 6 How Variable Stars get Their Names - D. Griffin .............................................. 9 References to Naming of Variable Stars - D. Griffin ........................................ 11 The Discovery of Three New Variable Stars using the Bradford Robotic Telescope and the Software Package Muniwin - D. Conner .................. 12 FY Librae - a First Look at the Behaviour during 2014 - P. Williams .............. 16 FY Librae goes Active and Reaffirms the Howarth and Bailey Formula - J. Toone .............. 18 Refining the Period of V505 Scuti - I. Miller ................................................... 21 Binocular Programme - M. Taylor ................................................................... 21 Eclipsing Binary Predictions – Where to Find Them - D. Loughney .............. 22 Charges for Section Publications .............................................. inside back cover Guidelines for Contributing to the Circular ............................. -
The Transfiguration in the Theology of Gregory Palamas And
Duquesne University Duquesne Scholarship Collection Electronic Theses and Dissertations Spring 2015 Deus in se et Deus pro nobis: The rT ansfiguration in the Theology of Gregory Palamas and Its Importance for Catholic Theology Cory Hayes Follow this and additional works at: https://dsc.duq.edu/etd Recommended Citation Hayes, C. (2015). Deus in se et Deus pro nobis: The rT ansfiguration in the Theology of Gregory Palamas and Its Importance for Catholic Theology (Doctoral dissertation, Duquesne University). Retrieved from https://dsc.duq.edu/etd/640 This Immediate Access is brought to you for free and open access by Duquesne Scholarship Collection. It has been accepted for inclusion in Electronic Theses and Dissertations by an authorized administrator of Duquesne Scholarship Collection. For more information, please contact [email protected]. DEUS IN SE ET DEUS PRO NOBIS: THE TRANSFIGURATION IN THE THEOLOGY OF GREGORY PALAMAS AND ITS IMPORTANCE FOR CATHOLIC THEOLOGY A Dissertation Submitted to the McAnulty Graduate School of Liberal Arts Duquesne University In partial fulfillment of the requirements for the degree of Doctor of Philosophy By Cory J. Hayes May 2015 Copyright by Cory J. Hayes 2015 DEUS IN SE ET DEUS PRO NOBIS: THE TRANSFIGURATION IN THE THEOLOGY OF GREGORY PALAMAS AND ITS IMPORTANCE FOR CATHOLIC THEOLOGY By Cory J. Hayes Approved March 31, 2015 _______________________________ ______________________________ Dr. Bogdan Bucur Dr. Radu Bordeianu Associate Professor of Theology Associate Professor of Theology (Committee Chair) (Committee Member) _______________________________ Dr. Christiaan Kappes Professor of Liturgy and Patristics Saints Cyril and Methodius Byzantine Catholic Seminary (Committee Member) ________________________________ ______________________________ Dr. James Swindal Dr. -
Australian Sky & Telescope
TRANSIT MYSTERY Strange sights BINOCULAR TOUR Dive deep into SHOOT THE MOON Take amazing as Mercury crosses the Sun p28 Virgo’s endless pool of galaxies p56 lunar images with your smartphone p38 TEST REPORT Meade’s 25-cm LX600-ACF P62 THE ESSENTIAL MAGAZINE OF ASTRONOMY Lasers and advanced optics are transforming astronomy p20 HOW TO BUY THE RIGHT ASTRO CAMERA p32 p14 ISSUE 93 MAPPING THE BIG BANG’S COSMIC ECHOES $9.50 NZ$9.50 INC GST LPI-GLPI-G LUNAR,LUNAR, PLANETARYPLANETARY IMAGERIMAGER ANDAND GUIDERGUIDER ASTROPHOTOGRAPHY MADE EASY. Let the LPI-G unleash the inner astrophotographer in you. With our solar, lunar and planetary guide camera, experience the universe on a whole new level. 0Image Sensor:'+(* C O LOR 0 Pixel Size / &#*('+ 0Frames per second/Resolution• / • / 0 Image Format: #,+$)!&))'!,# .# 0 Shutter%,*('#(%%#'!"-,,* 0Interface: 0Driver: ASCOM compatible 0GuiderPort: 0Color or Monochrome Models (&#'!-,-&' FEATURED DEALERS: MeadeTelescopes Adelaide Optical Centre | www.adelaideoptical.com.au MeadeInstrument The Binocular and Telescope Shop | www.bintel.com.au MeadeInstruments www.meade.com Sirius Optics | www.sirius-optics.com.au The device to free you from your handbox. With the Stella adapter, you can wirelessly control your GoTo Meade telescope at a distance without being limited by cord length. Paired with our new planetarium app, *StellaAccess, astronomers now have a graphical interface for navigating the night sky. STELLA WI-FI ADAPTER / $#)'$!!+#!+ #$#)'#)$##)$#'&*' / (!-')-$*')!($%)$$+' "!!$#$)(,#%',).( StellaAccess app. Available for use on both phones and tablets. /'$+((()$!'%!#)'*")($'!$)##!'##"$'$*) stars, planets, celestial bodies and more /$,'-),',### -' ($),' /,,,$"$')*!!!()$$"%)!)!($%( STELLA is controlled with Meade’s planetarium app, StellaAccess. Available for purchase for both iOS S and Android systems. -
Variable Star Classification and Light Curves Manual
Variable Star Classification and Light Curves An AAVSO course for the Carolyn Hurless Online Institute for Continuing Education in Astronomy (CHOICE) This is copyrighted material meant only for official enrollees in this online course. Do not share this document with others. Please do not quote from it without prior permission from the AAVSO. Table of Contents Course Description and Requirements for Completion Chapter One- 1. Introduction . What are variable stars? . The first known variable stars 2. Variable Star Names . Constellation names . Greek letters (Bayer letters) . GCVS naming scheme . Other naming conventions . Naming variable star types 3. The Main Types of variability Extrinsic . Eclipsing . Rotating . Microlensing Intrinsic . Pulsating . Eruptive . Cataclysmic . X-Ray 4. The Variability Tree Chapter Two- 1. Rotating Variables . The Sun . BY Dra stars . RS CVn stars . Rotating ellipsoidal variables 2. Eclipsing Variables . EA . EB . EW . EP . Roche Lobes 1 Chapter Three- 1. Pulsating Variables . Classical Cepheids . Type II Cepheids . RV Tau stars . Delta Sct stars . RR Lyr stars . Miras . Semi-regular stars 2. Eruptive Variables . Young Stellar Objects . T Tau stars . FUOrs . EXOrs . UXOrs . UV Cet stars . Gamma Cas stars . S Dor stars . R CrB stars Chapter Four- 1. Cataclysmic Variables . Dwarf Novae . Novae . Recurrent Novae . Magnetic CVs . Symbiotic Variables . Supernovae 2. Other Variables . Gamma-Ray Bursters . Active Galactic Nuclei 2 Course Description and Requirements for Completion This course is an overview of the types of variable stars most commonly observed by AAVSO observers. We discuss the physical processes behind what makes each type variable and how this is demonstrated in their light curves. Variable star names and nomenclature are placed in a historical context to aid in understanding today’s classification scheme. -
List of Easy Double Stars for Winter and Spring = Easy = Not Too Difficult = Difficult but Possible
List of Easy Double Stars for Winter and Spring = easy = not too difficult = difficult but possible 1. Sigma Cassiopeiae (STF 3049). 23 hr 59.0 min +55 deg 45 min This system is tight but very beautiful. Use a high magnification (150x or more). Primary: 5.2, yellow or white Seconary: 7.2 (3.0″), blue 2. Eta Cassiopeiae (Achird, STF 60). 00 hr 49.1 min +57 deg 49 min This is a multiple system with many stars, but I will restrict myself to the brightest one here. Primary: 3.5, yellow. Secondary: 7.4 (13.2″), purple or brown 3. 65 Piscium (STF 61). 00 hr 49.9 min +27 deg 43 min Primary: 6.3, yellow Secondary: 6.3 (4.1″), yellow 4. Psi-1 Piscium (STF 88). 01 hr 05.7 min +21 deg 28 min This double forms a T-shaped asterism with Psi-2, Psi-3 and Chi Piscium. Psi-1 is the uppermost of the four. Primary: 5.3, yellow or white Secondary: 5.5 (29.7), yellow or white 5. Zeta Piscium (STF 100). 01 hr 13.7 min +07 deg 35 min Primary: 5.2, white or yellow Secondary: 6.3, white or lilac (or blue) 6. Gamma Arietis (Mesarthim, STF 180). 01 hr 53.5 min +19 deg 18 min “The Ram’s Eyes” Primary: 4.5, white Secondary: 4.6 (7.5″), white 7. Lambda Arietis (H 5 12). 01 hr 57.9 min +23 deg 36 min Primary: 4.8, white or yellow Secondary: 6.7 (37.1″), silver-white or blue 8. -
Are Dust Shell Models Well-Suited to Explain Interferometric Data of Late
Astronomy & Astrophysics manuscript no. 3722 November 13, 2018 (DOI: will be inserted by hand later) Are dust shell models well-suited to explain interferometric data of late-type stars in the near-infrared? P. Schuller1,2, P. Salom´e3, G. Perrin4, B. Mennesson5, G. Niccolini6, P. de Laverny6, S.T. Ridgway7,4, V. Coud´edu Foresto4, and W.A. Traub2 1 Max-Planck-Institut f¨ur Astronomie, K¨onigstuhl 17, 69117 Heidelberg, Germany 2 Harvard-Smithsonian Center for Astrophysics, MS-20, 60 Garden Street, Cambridge, MA 02138, USA 3 Observatoire de Paris, LERMA, 61 Avenue de l’Observatoire, 75014 Paris, France 4 Observatoire de Paris, LESIA, 5 Place Jules Janssen, 92195 Meudon, France 5 Jet Propulsion Laboratory, MS 306-388, 4800 Oak Grove Drive, Pasadena, CA 91109, USA 6 Observatoire de la Cˆote d’Azur, D´epartement Fresnel UMR 6528, BP 4229, 06304 Nice, France 7 National Optical Astronomy Observatories, P.O. Box 26732, Tucson, AZ 85726, USA Received ... / accepted ... Abstract. Recently available near-infrared interferometric data on late-type stars show a strong increase of diameter for asymp- totic giant branch (AGB) stars between the K (2.0 − 2.4 µm) and L (3.4 − 4.1 µm) bands. Aiming at an explanation of these findings, we chose the objects α Orionis (Betelgeuse), SW Virginis, and R Leonis, which are of different spectral types and stages of evolution, and which are surrounded by circumstellar envelopes with different optical thicknesses. For these stars, we compared observations with spherically symmetric dust shell models. Photometric and 11 µm interferometric data were also taken into account to further constrain the models. -
April 14 2018 7:00Pm at the April 2018 Herrett Center for Arts & Science College of Southern Idaho
Snake River Skies The Newsletter of the Magic Valley Astronomical Society www.mvastro.org Membership Meeting President’s Message Tim Frazier Saturday, April 14th 2018 April 2018 7:00pm at the Herrett Center for Arts & Science College of Southern Idaho. It really is beginning to feel like spring. The weather is more moderate and there will be, hopefully, clearer skies. (I write this with some trepidation as I don’t want to jinx Public Star Party Follows at the it in a manner similar to buying new equipment will ensure at least two weeks of Centennial Observatory cloudy weather.) Along with the season comes some great spring viewing. Leo is high overhead in the early evening with its compliment of galaxies as is Coma Club Officers Berenices and Virgo with that dense cluster of extragalactic objects. Tim Frazier, President One of my first forays into the Coma-Virgo cluster was in the early 1960’s with my [email protected] new 4 ¼ inch f/10 reflector and my first star chart, the epoch 1960 version of Norton’s Star Atlas. I figured from the maps I couldn’t miss seeing something since Robert Mayer, Vice President there were so many so closely packed. That became the real problem as they all [email protected] appeared as fuzzy spots and the maps were not detailed enough to distinguish one galaxy from another. I still have that atlas as it was a precious Christmas gift from Gary Leavitt, Secretary my grandparents but now I use better maps, larger scopes and GOTO to make sure [email protected] it is M84 or M86. -
Double and Multiple Star Measurements in the Northern Sky with a 10” Newtonian and a Fast CCD Camera in 2006 Through 2009
Vol. 6 No. 3 July 1, 2010 Journal of Double Star Observations Page 180 Double and Multiple Star Measurements in the Northern Sky with a 10” Newtonian and a Fast CCD Camera in 2006 through 2009 Rainer Anton Altenholz/Kiel, Germany e-mail: rainer.anton”at”ki.comcity.de Abstract: Using a 10” Newtonian and a fast CCD camera, recordings of double and multiple stars were made at high frame rates with a notebook computer. From superpositions of “lucky images”, measurements of 139 systems were obtained and compared with literature data. B/w and color images of some noteworthy systems are also presented. mented double stars, as will be described in the next Introduction section. Generally, I used a red filter to cope with By using the technique of “lucky imaging”, seeing chromatic aberration of the Barlow lens, as well as to effects can strongly be reduced, and not only the reso- reduce the atmospheric spectrum. For systems with lution of a given telescope can be pushed to its limits, pronounced color contrast, I also made recordings but also the accuracy of position measurements can be with near-IR, green and blue filters in order to pro- better than this by about one order of magnitude. This duce composite images. This setup was the same as I has already been demonstrated in earlier papers in used with telescopes under the southern sky, and as I this journal [1-3]. Standard deviations of separation have described previously [1-3]. Exposure times varied measurements of less than +/- 0.05 msec were rou- between 0.5 msec and 100 msec, depending on the tinely obtained with telescopes of 40 or 50 cm aper- star brightness, and on the seeing. -
Meteor 23. Évf. 6. Sz. (1993.)
ROVATVEZETŐINK: ■ NAP Iskum József meteor Budapest, Rózsa u. 48. 1041 ■ HOLD A Magyar Csillagászati Egyesület Kocsis Antal lapja Balatonkenese, Kossuth u. 2/a. 8174 Journal of the Hungarian Astronomical Association ■ BOLYGÓK Vincze Iván Redaction: Pécs, Aidinger J. u. 15. 7632 H-1461 Budapest, P.0. Box 219, Hungary ■ ÜSTÖKÖSÖK HU ISSN 0133-249X Sárneczky Krisztián Budapest, Kádár u. 9-11. 1132 Tel.: (1)-153-4902 A Meteor előfizetési díja 1993-ra ■ METEOROK (nem tagok számára) 800 Ft + ÁFA Tepliczky István Tata, Baji út 42. 2890 Évközben i előfizetés (tagdíjbefizetés) ■ CSILLAGFEDÉSEK esetén a számokat visszamenőleg Szabó Sándor megküldjük. Sopron, Baross u. 12. 9400 ■ KETTŐSCSILLAGOK Főszerkesztő: Ladányi Tamás Mizser Attila Balatonfűzfő, Balaton krt. 71. 8175 Tel.: (80J-51-744 Olvasószerkesztők: ■ VÁLTOZÓCSILLAGOK Csaba György Gábor Mizser Attila Dr. Kolláth Zoltán Budapest, Pf. 219. 1461 Tepliczky István Tel.: (1 )-186-2313 ■ MÉLY-ÉG OBJEKTUMOK A Magyar Csillagászati Egyesület és a Papp Sándor szerkesztőség postacíme: Kecskemét, Csokonai u. 1. 6000 Budapest, Pf. 219. 1461 ■ MESSIER KLUB Nagy Zoltán Antal Felelős kiadó az MCSE elnöke. Budapest, Corvin krt. 49. 1192 Megjelenik ■ SZABADSZEMES JELENSÉGEK a Pro Renovadna Cultura Hungáriáé Keresztúri Ákos Alapítvány támogatásával Budapest, Komjády B. u. 1. 1023 Tel.: (1)-115-6772 ■ CSILLAGÁSZATTÖRTÉNET Keszthelyi Sándor MAGYAR Pécs, Alkotmány u. 3. 7624 CSILLAGÁSZATI ■ TÁVCSŐKÉSZÍTÉS EGYESÜLET Dán András Az egyesületi tagság formái (1993): Etyek, Alsóhegy u. 7. 2091 — rendes tagsági díj (illetmény: ■ SZÁMÍTÁSTECHNIKA Meteor csili, évkönyv) 600 Ft Heitler Gábor Piliscsaba, Egyetem út 5. 2081 — pártoló tagsági díj (ill.: Meteor + Meteor csili, évkönyv) 1200 Ft A BESZÁMOLÓK BEKÜLDÉSE — örökös pártoló tagdíj 30000 Ft MINDEN HÓ 6-áig! Tartalom Contents XXIII. -
Read Full Text (PDF)
Gas infall and possible circumstellar rotation in R Leonis Downloaded from: https://research.chalmers.se, 2021-10-02 00:25 UTC Citation for the original published paper (version of record): Fonfria, J., Santander-Garcia, M., Cernicharo, J. et al (2019) Gas infall and possible circumstellar rotation in R Leonis Astronomy and Astrophysics, 622 http://dx.doi.org/10.1051/0004-6361/201834840 N.B. When citing this work, cite the original published paper. research.chalmers.se offers the possibility of retrieving research publications produced at Chalmers University of Technology. It covers all kind of research output: articles, dissertations, conference papers, reports etc. since 2004. research.chalmers.se is administrated and maintained by Chalmers Library (article starts on next page) A&A 622, L14 (2019) Astronomy https://doi.org/10.1051/0004-6361/201834840 & c ESO 2019 Astrophysics LETTER TO THE EDITOR Gas infall and possible circumstellar rotation in R Leonis? J. P. Fonfría1, M. Santander-García2, J. Cernicharo1, L. Velilla-Prieto3, M. Agúndez1, N. Marcelino1, and G. Quintana-Lacaci1 1 Molecular Astrophysics Group, Instituto de Física Fundamental, CSIC, C/ Serrano, 123, 28006 Madrid, Spain e-mail: [email protected] 2 Observatorio Astronómico Nacional, OAN-IGN, Alfonso XII, 3, 28014 Madrid, Spain 3 Dept. of Space, Earth, and Environment, Astronomy and Plasma Physics Division, Chalmers University of Technology, Onsala Space Observatory, 439 92 Onsala, Sweden Received 12 December 2018 / Accepted 6 February 2019 ABSTRACT We present new interferometer molecular observations of R Leo taken at 1.2 mm with the Atacama Large Millimeter Array with an angular resolution up to '000: 026.