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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. -
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. -
GTO Keypad Manual, V5.001
ASTRO-PHYSICS GTO KEYPAD Version v5.xxx Please read the manual even if you are familiar with previous keypad versions Flash RAM Updates Keypad Java updates can be accomplished through the Internet. Check our web site www.astro-physics.com/software-updates/ November 11, 2020 ASTRO-PHYSICS KEYPAD MANUAL FOR MACH2GTO Version 5.xxx November 11, 2020 ABOUT THIS MANUAL 4 REQUIREMENTS 5 What Mount Control Box Do I Need? 5 Can I Upgrade My Present Keypad? 5 GTO KEYPAD 6 Layout and Buttons of the Keypad 6 Vacuum Fluorescent Display 6 N-S-E-W Directional Buttons 6 STOP Button 6 <PREV and NEXT> Buttons 7 Number Buttons 7 GOTO Button 7 ± Button 7 MENU / ESC Button 7 RECAL and NEXT> Buttons Pressed Simultaneously 7 ENT Button 7 Retractable Hanger 7 Keypad Protector 8 Keypad Care and Warranty 8 Warranty 8 Keypad Battery for 512K Memory Boards 8 Cleaning Red Keypad Display 8 Temperature Ratings 8 Environmental Recommendation 8 GETTING STARTED – DO THIS AT HOME, IF POSSIBLE 9 Set Up your Mount and Cable Connections 9 Gather Basic Information 9 Enter Your Location, Time and Date 9 Set Up Your Mount in the Field 10 Polar Alignment 10 Mach2GTO Daytime Alignment Routine 10 KEYPAD START UP SEQUENCE FOR NEW SETUPS OR SETUP IN NEW LOCATION 11 Assemble Your Mount 11 Startup Sequence 11 Location 11 Select Existing Location 11 Set Up New Location 11 Date and Time 12 Additional Information 12 KEYPAD START UP SEQUENCE FOR MOUNTS USED AT THE SAME LOCATION WITHOUT A COMPUTER 13 KEYPAD START UP SEQUENCE FOR COMPUTER CONTROLLED MOUNTS 14 1 OBJECTS MENU – HAVE SOME FUN! -
Arxiv:2006.10868V2 [Astro-Ph.SR] 9 Apr 2021 Spain and Institut D’Estudis Espacials De Catalunya (IEEC), C/Gran Capit`A2-4, E-08034 2 Serenelli, Weiss, Aerts Et Al
Noname manuscript No. (will be inserted by the editor) Weighing stars from birth to death: mass determination methods across the HRD Aldo Serenelli · Achim Weiss · Conny Aerts · George C. Angelou · David Baroch · Nate Bastian · Paul G. Beck · Maria Bergemann · Joachim M. Bestenlehner · Ian Czekala · Nancy Elias-Rosa · Ana Escorza · Vincent Van Eylen · Diane K. Feuillet · Davide Gandolfi · Mark Gieles · L´eoGirardi · Yveline Lebreton · Nicolas Lodieu · Marie Martig · Marcelo M. Miller Bertolami · Joey S.G. Mombarg · Juan Carlos Morales · Andr´esMoya · Benard Nsamba · KreˇsimirPavlovski · May G. Pedersen · Ignasi Ribas · Fabian R.N. Schneider · Victor Silva Aguirre · Keivan G. Stassun · Eline Tolstoy · Pier-Emmanuel Tremblay · Konstanze Zwintz Received: date / Accepted: date A. Serenelli Institute of Space Sciences (ICE, CSIC), Carrer de Can Magrans S/N, Bellaterra, E- 08193, Spain and Institut d'Estudis Espacials de Catalunya (IEEC), Carrer Gran Capita 2, Barcelona, E-08034, Spain E-mail: [email protected] A. Weiss Max Planck Institute for Astrophysics, Karl Schwarzschild Str. 1, Garching bei M¨unchen, D-85741, Germany C. Aerts Institute of Astronomy, Department of Physics & Astronomy, KU Leuven, Celestijnenlaan 200 D, 3001 Leuven, Belgium and Department of Astrophysics, IMAPP, Radboud University Nijmegen, Heyendaalseweg 135, 6525 AJ Nijmegen, the Netherlands G.C. Angelou Max Planck Institute for Astrophysics, Karl Schwarzschild Str. 1, Garching bei M¨unchen, D-85741, Germany D. Baroch J. C. Morales I. Ribas Institute of· Space Sciences· (ICE, CSIC), Carrer de Can Magrans S/N, Bellaterra, E-08193, arXiv:2006.10868v2 [astro-ph.SR] 9 Apr 2021 Spain and Institut d'Estudis Espacials de Catalunya (IEEC), C/Gran Capit`a2-4, E-08034 2 Serenelli, Weiss, Aerts et al. -
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. -
The Survey of Western Palestine. a General Index
THE SURVEY OF WESTERN PALESTINE. A GENERAL INDEX TO 1. THE MEMOIRS, VOLS. I.-III. 2. THE SPECIAL PAPERS. 3. THE JERUSALEM VOLUME. 4. THE FLORA AND FAUNA OF PALESTINE. 5. THE GEOLOGICAL SURVEY. AND TO THE ARABIC AND ENGLISH NAME LISTS. COMPILED BY HENRY C. STEWARDSON. 1888 Electronic Edition by Todd Bolen BiblePlaces.com 2005 PREFACE. ITTLE explanation is required of the arrangement followed in this Volume, beyond calling L attention to the division of this Volume into two parts: the first forms a combined Index to the three Volumes of the Memoirs, the Special Papers, the Jerusalem Volume, the Flora and Fauna of Palestine, and the Geological Survey; and the second is an Index to the Arabic and English Name Lists. This division was considered advisable in order to avoid the continual use of reference letters to the Name Lists, which would otherwise have been required. The large number of entries rendered it absolutely necessary to make them as brief as possible; but it is hoped that it will be found that perspicuity has not been sacrificed to brevity. A full explanation of the reference letters used will be found on the first page. The short Hebrew Index at the end of the Volume has been kindly furnished by Dr. W. Aldis Wright. H. C. S. PREFACE TO ELECTRONIC EDITION. ore than a hundred years after the publication of the Survey of Western Palestine, its M continued value is well-known and is evidenced by the recent reprint and librarians’ propensity to store the work in restricted areas of the library. -
1 I Articles Dans Des Revues Avec Comité De Lecture
1 I Articles dans des revues avec comité de lecture (ACL) internationales II Articles dans des revues sans comité de lecture (SCL) NB : La liste des publications est donnée de façon exhautive par équipe, ce qui signifie qu’il existe des redondances chaque fois qu’une publication est cosignée pas des membres dépendant d’équipes différentes. Par contre, certains chercheurs sont à cheval sur deux équipes, dans ce cas il leur a été demandé de rattacher leurs publications seulement à l’une ou à l’autre équipe en fonction de la nature de la publication et la raison de leur rattachement à deux équipes. I Articles dans des revues avec comité de lecture (ACL) internationales ANNÉE 2006 A / Equipe « Physique des galaxies » 1. Aguilar, J.A. et al. (the ANTARES collaboration, 214 auteurs). First results of the Instrumentation Line for the deep- sea ANTARES neturino telescope Astroparticle Physic 26, 314 2. Auld, R.; Minchin, R. F.; Davies, J. I.; Catinella, B.; van Driel, W.; Henning, P. A.; Linder, S.; Momjian, E.; Muller, E.; O'Neil, K.; Boselli, A.; et 18 coauteurs. The Arecibo Galaxy Environment Survey: precursor observations of the NGC 628 group, 2006, MNRAS,.371,1617A 3. Boselli, A.; Boissier, S.; Cortese, L.; Gil de Paz, A.; Seibert, M.; Madore, B. F.; Buat, V.; Martin, D. C. The Fate of Spiral Galaxies in Clusters: The Star Formation History of the Anemic Virgo Cluster Galaxy NGC 4569, 2006, ApJ, 651, 811B 4. Boselli, A.; Gavazzi, G. Environmental Effects on Late-Type Galaxies in Nearby Clusters -2006, PASP, 118, 517 5. -
Statistics and Supermetallicity: the Metallicity of Mu Leonis
A&A 379, 917–923 (2001) Astronomy DOI: 10.1051/0004-6361:20011380 & c ESO 2001 Astrophysics Statistics and supermetallicity: The metallicity of Mu Leonis B. J. Taylor? Department of Physics and Astronomy, N283 ESC, Brigham Young University, Provo, UT 84602-4360, USA Received 9 February 2001 / Accepted 2 October 2001 Abstract. For the often-studied “SMR” giant µ Leo, Smith & Ruck (2000) have recently found that [Fe/H] ∼ +0.3 dex. Their conclusion is tested here in a “statistical” paradigm, in which statistical principles are used to select published high-dispersion µ Leo data and assign error bars to them. When data from Smith & Ruck and from Takeda et al. (1998) are added to a data base compiled in 1999, it is found that conclusions from an earlier analysis (Taylor 1999c) are essentially unchanged: the mean value of [Fe/H] ∼ +0.23 0.025 dex, and values ≤+0.2 dex are not clearly ruled out at 95% confidence. In addition, the hypothesis that [Fe/H] ≥ +0.3dexwhich emerges from the Smith-Ruck analysis is formally rejected at 98% confidence. The “default paradigm” which is commonly used to assess µ Leo data is also considered. The basic characteristics of that paradigm continue to be a) unexplained exclusion of statistical analysis, b) inadequately explained deletions from an [Fe/H] data base containing accordant data, and c) an undefended convention that µ Leo is to have a metallicity of about +0.3dex or higher. As a result, it seems fair to describe the Smith-Ruck application and other applications of the default paradigm as invalid methods of inference from the data. -
April 2016 BRAS Newsletter
April 2016 Issue th Next Meeting: Monday, April 11 at 7PM at HRPO (2nd Mondays, Highland Road Park Observatory) April 6th through April 10th is our annual Hodges Gardens Star Party. You can pre-register using the form on the BRAS website. If you have never attended this star party, make plans to attend this one. What's In This Issue? President’s Message Photos: BRAS Telescope donated to EBRP Library Secretary's Summary of March Meeting Recent BRAS Forum Entries 20/20 Vision Campaign Message from the HRPO Astro Short: Stellar Dinosaurs? International Astronomy Day Observing Notes: Leo The Lion, by John Nagle Newsletter of the Baton Rouge Astronomical Society April 2016 Page 2 President’s Message There were 478 people who stopped by the BRAS display at the March 19th ―Rockin at the Swamp‖ event at the Bluebonnet Swamp and Nature Center. I give thanks to all our volunteers for our success in this outreach event. April 6th through April 10th is our annual Hodges Gardens Star Party. You can pre-register on the BRAS website, or register when you arrive (directions are on the BRAS website). If you have never attended a star party, of if you are an old veteran star partier; make plans to attend this one. Our Guest Speaker for the BRAS meeting on April 11th will be Dr. Joseph Giaime, Observatory Head, LIGO Livingston (Caltech), Professor of Physics and Astronomy (LSU). Yes, he will be talking about gravity waves and the extraordinary discovery LIGO has made. We need volunteers to help at our display on Earth Day on Sunday, April 17th. -
Bibliography from ADS File: Lambert.Bib August 16, 2021 1
Bibliography from ADS file: lambert.bib Reddy, A. B. S. & Lambert, D. L., “VizieR Online Data Cata- August 16, 2021 log: Abundance ratio for 5 local stellar associations (Reddy+, 2015)”, 2018yCat..74541976R ADS Reddy, A. B. S., Giridhar, S., & Lambert, D. L., “VizieR Online Data Deepak & Lambert, D. L., “Lithium in red giants: the roles of the He-core flash Catalog: Line list for red giants in open clusters (Reddy+, 2015)”, and the luminosity bump”, 2021arXiv210704624D ADS 2017yCat..74504301R ADS Deepak & Lambert, D. L., “Lithium in red giants: the roles of the He-core flash Ramírez, I., Yong, D., Gutiérrez, E., et al., “Iota Horologii Is Unlikely to Be an and the luminosity bump”, 2021MNRAS.tmp.1807D ADS Evaporated Hyades Star”, 2017ApJ...850...80R ADS Deepak & Lambert, D. L., “Lithium abundances and asteroseismology of red gi- Ramya, P., Reddy, B. E., Lambert, D. L., & Musthafa, M. M., “VizieR On- ants: understanding the evolution of lithium in giants based on asteroseismic line Data Catalog: Hercules stream K giants analysis (Ramya+, 2016)”, parameters”, 2021MNRAS.505..642D ADS 2017yCat..74601356R ADS Federman, S. R., Rice, J. S., Ritchey, A. M., et al., “The Transition Hema, B. P., Pandey, G., Kamath, D., et al., “Abundance Analyses of from Diffuse Molecular Gas to Molecular Cloud Material in Taurus”, the New R Coronae Borealis Stars: ASAS-RCB-8 and ASAS-RCB-10”, 2021ApJ...914...59F ADS 2017PASP..129j4202H ADS Bhowmick, A., Pandey, G., & Lambert, D. L., “Fluorine detection in hot extreme Pandey, G. & Lambert, D. L., “Non-local Thermodynamic Equilibrium Abun- helium stars”, 2020JApA...41...40B ADS dance Analyses of the Extreme Helium Stars V652 Her and HD 144941”, Reddy, A. -
Basics of Astrophysics Revisited. I. Mass- Luminosity Relation for K, M and G Class Stars
Basics of astrophysics revisited. I. Mass- luminosity relation for K, M and G class stars Edgars Alksnis [email protected] Small volume statistics show, that luminosity of slow rotating stars is proportional to their angular momentums of rotation. Cause should be outside of standard solar model. Slow rotating giants and dim dwarfs are not out of „main sequence” in this concept. Predictive power of stellar mass-radius- equatorial rotation speed-luminosity relation has been offered to test in numerous examples. Keywords: mass-luminosity relation, stellar rotation, stellar mass prediction, stellar rotation prediction ...Such vibrations would proceed from deep inside the sun. They are a fast way of transporting large amounts of energy from the interior to the surface that is not envisioned in present theory.... They could stir up the material inside the sun, which current theory tends to see as well layered, and that could affect the fusion dynamics. If they come to be generally accepted, they will require a reworking of solar theory, and that carries in its train a reworking of stellar theory generally. These vibrations could reverberate throughout astronomy. (Science News, Vol. 115, April 21, 1979, p. 270). Actual expression for stellar mass-luminosity relation (fig.1) Fig.1 Stellar mass- luminosity relation. Credit: Ay20. L- luminosity, relative to the Sun, M- mass, relative to the Sun. remain empiric and in fact contain unresolvable contradiction: stellar luminosity basically is connected with their surface area (radius squared) but mass (radius in cube) appears as a factor which generate luminosity. That purely geometric difference had pressed astrophysicists to place several classes of stars outside of „main sequence” in the frame of their strange theoretic constructions. -
Milestone Goto-Bino Series .Cdr
Kson MilestoneK Standard Alt/Az GOTO Mount INSTRUCTIONS CONTENT FOR KSON STANDARD ALT/AZ GOTO USER INTRODUCTION.................................................................................1 ACCESSORIES..................................................................................2 ASSEMBLY INSTRUCTIONS.............................................................3 FEATURES.........................................................................5 OPERATION MANUAL FOR SKYTOUCH CONTROLLER............... 6 KEY DESCRIPTION.................................................................................6 STATUS DESCRIPTION...........................................................................6 OPERATION PROCESS...........................................................................7 POWER ON......................................................................................7 WARNING........................................................................................7 ALIGNMENT STATUS........................................................................7 CHANGE THE DATE..................................................................7 CHANGE THE TIME...................................................................8 CHANGE THE SITE...................................................................8 ALIGNMENT.............................................................................9 NAVIGATION STATUS.....................................................................11 MENU STATUS................................................................................11