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13076197 Tanvir Tabassum Final Version of Submission.Pdf
Finding Close Encounters: Toward a consensus on the influence of the stellar flybys on the Solar System over 10 million years Supervised by: Author: Dr Fabo Feng Tabassum Shahriar Tanvir Dr James L Collett Professor Hugh Jones Centre for Astrophysics Research School of Physics, Astronomy and Mathematics University of Hertfordshire Submitted to the University of Hertfordshire in partial fulfilment of the requirements of the degree of Master of Science by Research. October 2018 Abstract This thesis is a study of possible stellar encounters of the Sun, both in the past and in the future within ±10 Myr of the current epoch. This study is based on data gleaned from the first Gaia data release (Gaia DR1). One of the components of the Gaia DR1 is the TGAS catalogue. TGAS contained five astrometric parameters for more than two million stars. Four separate catalogues were used to provide radial velocities for these stars. A linear motion approximation was used to make a cut within an initial catalogue keeping only the stars that would have perihelia within 10 pc. 1003 stars were found to have a perihelion distance less than 10 pc. Each of these stars was then cloned 1000 times from their covariance matrix from Gaia DR1. The stars’ orbits were numerically integrated through a model galactic potential. After the integration, a particularly interesting set of candidates was selected for deeper study. In particular stars with a mean perihelion distance less than 2 pc were chosen for a deeper study since they will have significant influence on the Oort cloud. 46 stars were found to have a mean perihelion distance less than 2 pc. -
MARS an Overview of the 1985–2006 Mars Orbiter Camera Science
MARS MARS INFORMATICS The International Journal of Mars Science and Exploration Open Access Journals Science An overview of the 1985–2006 Mars Orbiter Camera science investigation Michael C. Malin1, Kenneth S. Edgett1, Bruce A. Cantor1, Michael A. Caplinger1, G. Edward Danielson2, Elsa H. Jensen1, Michael A. Ravine1, Jennifer L. Sandoval1, and Kimberley D. Supulver1 1Malin Space Science Systems, P.O. Box 910148, San Diego, CA, 92191-0148, USA; 2Deceased, 10 December 2005 Citation: Mars 5, 1-60, 2010; doi:10.1555/mars.2010.0001 History: Submitted: August 5, 2009; Reviewed: October 18, 2009; Accepted: November 15, 2009; Published: January 6, 2010 Editor: Jeffrey B. Plescia, Applied Physics Laboratory, Johns Hopkins University Reviewers: Jeffrey B. Plescia, Applied Physics Laboratory, Johns Hopkins University; R. Aileen Yingst, University of Wisconsin Green Bay Open Access: Copyright 2010 Malin Space Science Systems. This is an open-access paper distributed under the terms of a Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited. Abstract Background: NASA selected the Mars Orbiter Camera (MOC) investigation in 1986 for the Mars Observer mission. The MOC consisted of three elements which shared a common package: a narrow angle camera designed to obtain images with a spatial resolution as high as 1.4 m per pixel from orbit, and two wide angle cameras (one with a red filter, the other blue) for daily global imaging to observe meteorological events, geodesy, and provide context for the narrow angle images. Following the loss of Mars Observer in August 1993, a second MOC was built from flight spare hardware and launched aboard Mars Global Surveyor (MGS) in November 1996. -
Making a Game Character Move
Piia Brusi MAKING A GAME CHARACTER MOVE Animation and motion capture for video games Bachelor’s thesis Degree programme in Game Design 2021 Author (authors) Degree title Time Piia Brusi Bachelor of Culture May 2021 and Arts Thesis title 69 pages Making a game character move Animation and motion capture for video games Commissioned by South Eastern Finland University of Applied Sciences Supervisor Marko Siitonen Abstract The purpose of this thesis was to serve as an introduction and overview of video game animation; how the interactive nature of games differentiates game animation from cinematic animation, what the process of producing game animations is like, what goes into making good game animations and what animation methods and tools are available. The thesis briefly covered other game design principles most relevant to game animators: game design, character design, modelling and rigging and how they relate to game animation. The text mainly focused on animation theory and practices based on commentary and viewpoints provided by industry professionals. Additionally, the thesis described various 3D animation and motion capture systems and software in detail, including how motion capture footage is shot and processed for games. The thesis ended on a step-by-step description of the author’s motion capture cleanup project, where a jog loop was created out of raw motion capture data. As the topic of game animation is vast, the thesis could not cover topics such as facial motion capture and procedural animation in detail. Technologies such as motion matching, machine learning and range imaging were also suggested as topics worth covering in the future. -
RATIOS and STAR FORMATION EFFICIENCIES in SUPERGIANT H Ii REGIONS
The Astrophysical Journal, 788:167 (7pp), 2014 June 20 doi:10.1088/0004-637X/788/2/167 C 2014. The American Astronomical Society. All rights reserved. Printed in the U.S.A. ENHANCEMENT OF CO(3–2)/CO(1–0) RATIOS AND STAR FORMATION EFFICIENCIES IN SUPERGIANT H ii REGIONS Rie E. Miura1,2, Kotaro Kohno3,4, Tomoka Tosaki5, Daniel Espada1,6,7, Akihiko Hirota8, Shinya Komugi1, Sachiko K. Okumura9, Nario Kuno7,8, Kazuyuki Muraoka10, Sachiko Onodera10, Kouichiro Nakanishi1,6,7, Tsuyoshi Sawada1,6, Hiroyuki Kaneko11, Tetsuhiro Minamidani8, Kosuke Fujii1,2, and Ryohei Kawabe1,6 1 National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan; [email protected] 2 Department of Astronomy, The University of Tokyo, Hongo, Bunkyo-ku, Tokyo 133-0033, Japan 3 Institute of Astronomy, School of Science, The University of Tokyo, Osawa, Mitaka, Tokyo 181-0015, Japan 4 Research Center for Early Universe, School of Science, The University of Tokyo, Hongo, Bunkyo, Tokyo 113-0033, Japan 5 Joetsu University of Education, Yamayashiki-machi, Joetsu, Niigata 943-8512, Japan 6 Joint ALMA Observatory, Alonso de Cordova 3107, Vitacura 763-0355, Santiago, Chile 7 Department of Astronomical Science, The Graduate University for Advanced Studies (Sokendai), 2-21-1 Osawa, Mitaka, Tokyo 181-0015, Japan 8 Nobeyama Radio Observatory, Minamimaki, Minamisaku, Nagano 384-1805, Japan 9 Department of Mathematical and Physical Sciences, Faculty of Science, Japan Woman’s University, Mejirodai 2-8-1, Bunkyo, Tokyo 112-8681, Japan 10 Osaka Prefecture University, -
Tvorba Interaktivního Animovaného Příběhu
Středoškolská technika 2014 Setkání a prezentace prací středoškolských studentů na ČVUT Tvorba interaktivního animovaného příběhu Sami Salama Střední průmyslová škola na Proseku Novoborská 2, 190 00 Praha 9 1 Obsah 1 Obsah .................................................................................................................. 1 2 2D grafika (základní pojmy) ................................................................................. 3 2.1 Základní vysvětlení pojmu (počítačová) 2D grafika ....................................... 3 2.2 Rozdíl - 2D vs. 3D grafika .............................................................................. 3 2.3 Vektorová grafika ........................................................................................... 4 2.4 Rastrová grafika ............................................................................................ 6 2.5 Výhody a nevýhody rastrové grafiky .............................................................. 7 2.6 Rozlišení ........................................................................................................ 7 2.7 Barevná hloubka............................................................................................ 8 2.8 Základní grafické formáty .............................................................................. 8 2.9 Druhy komprese dat ...................................................................................... 9 2.10 Barevný model .......................................................................................... -
From Luminous Hot Stars to Starburst Galaxies
9780521791342pre CUP/CONT July 9, 2008 11:48 Page-i FROM LUMINOUS HOT STARS TO STARBURST GALAXIES Luminous hot stars represent the extreme upper mass end of normal stellar evolution. Before exploding as supernovae, they live out their lives of only a few million years with prodigious outputs of radiation and stellar winds which dramatically affect both their evolution and environments. A detailed introduction to the topic, this book connects the astrophysics of mas- sive stars with the extremes of galaxy evolution represented by starburst phenomena. A thorough discussion of the physical and wind parameters of massive stars is pre- sented, together with considerations of their birth, evolution, and death. Hll galaxies, their connection to starburst galaxies, and the contribution of starburst phenomena to galaxy evolution through superwinds, are explored. The book concludes with the wider cosmological implications, including Population III stars, Lyman break galaxies, and gamma-ray bursts, for each of which massive stars are believed to play a crucial role. This book is ideal for graduate students and researchers in astrophysics who are interested in massive stars and their role in the evolution of galaxies. Peter S. Conti is an Emeritus Professor at the Joint Institute for Laboratory Astro- physics (JILA) and theAstrophysics and Planetary Sciences Department at the University of Colorado. Paul A. Crowther is a Professor of Astrophysics in the Department of Physics and Astronomy at the University of Sheffield. Claus Leitherer is an Astronomer with the Space Telescope Science Institute, Baltimore. 9780521791342pre CUP/CONT July 9, 2008 11:48 Page-ii Cambridge Astrophysics Series Series editors: Andrew King, Douglas Lin, Stephen Maran, Jim Pringle and Martin Ward Titles available in the series 10. -
In-Depth Study of Photometric Variability and Radiative Timescales for Atmospheric Evolution in Four L Dwarfs
Weather on Other Worlds IV: In-Depth Study of Photometric Variability and Radiative Timescales for Atmospheric Evolution in Four L Dwarfs Item Type text; Electronic Thesis Authors Flateau, Davin C. Publisher The University of Arizona. Rights Copyright © is held by the author. Digital access to this material is made possible by the University Libraries, University of Arizona. Further transmission, reproduction or presentation (such as public display or performance) of protected items is prohibited except with permission of the author. Download date 30/09/2021 07:25:39 Link to Item http://hdl.handle.net/10150/594630 WEATHER ON OTHER WORLDS IV: IN-DEPTH STUDY OF PHOTOMETRIC VARIABILITY AND RADIATIVE TIMESCALES FOR ATMOSPHERIC EVOLUTION IN FOUR L DWARFS by Davin C. Flateau A Thesis Submitted to the Faculty of the DEPARTMENT OF PLANETARY SCIENCES In Partial Fulfillment of the Requirements For the Degree of MASTER OF SCIENCE In the Graduate College THE UNIVERSITY OF ARIZONA 2015 2 STATEMENT BY AUTHOR This thesis has been submitted in partial fulfillment of requirements for an advanced degree at the University of Arizona and is deposited in the University Library to be made available to borrowers under rules of the Library. Brief quotations from this thesis are allowable without special permission, provided that accurate acknowledgment of the source is made. Requests for permission for extended quotation from or reproduction of this manuscript in whole or in part may be granted by the head of the major department or the Dean of the Graduate College when in his or her judgment the proposed use of the material is in the interests of scholarship. -
DOUBLE STARS INFORMATION CIRCULAR No. 202 (OCTOBER 2020)
INTERNATIONAL ASTRONOMICAL UNION COMMISSION G1 (BINARY AND MULTIPLE STAR SYSTEMS) DOUBLE STARS INFORMATION CIRCULAR No. 202 (OCTOBER 2020) NEW ORBITS ADS Name P T e Ω(2000) 2020 Author(s) α2000δ n a i ! Last ob. 2021 1762 A 207 1204y6 1937.27 0.816 31◦3 358◦9 000629 SCARDIA 02182+3920 0◦2989 000950 31◦1 193◦9 2020.771 359.2 0.635 et al. (*) 1477 WRH 39 Aa,Ab 29.59 1987.66 0.608 189.5 327.3 0.081 DOCOBO 02318+8916 12.1663 0.120 146.2 123.0 2014.4856 312.1 0.093 & CAMPO - COU 1688 AB 8.638 2003.841 0.198 49.2 247.6 0.121 DOCOBO 03321+4340 41.6763 0.139 35.5 268.2 2012.7023 308.0 0.092 & LING 3303 HU 1082 53.17 2023.24 0.746 108.9 221.1 0.151 DOCOBO 04349+3908 6.7707 0.362 48.9 216.3 2007.8019 240.7 0.132 & LING 3730 BU 1047 BC 34.38 2001.21 0.944 30.9 78.1 0.357 DOCOBO 05098+2802 10.4712 0.282 122.4 114.9 2007.8184 77.0 0.357 & CAMPO 11635 STF 2382 AB 2802.8 2051.49 0.953 149.6 344.3 2.169 DOCOBO 18443+3940 0.1284 14.237 102.2 258.8 2020.7470 344.0 2.148 & CAMPO 11635 STF 2383 CD 724.3 2223.9 0.353 26.5 74.3 2.399 DOCOBO 18443+3940 0.4970 2.920 126.1 73.8 2020.7470 73.9 2.402 & CAMPO 11635 CHR 77 Ca,Cb 15.75 2008.94 0.411 42.4 48.2 0.229 DOCOBO 18443+3940 22.8571 0.191 109.9 127.2 2005.5155 42.9 0.214 & CAMPO 13950 COU 1962 AB 20.414 1999.240 0.524 116.7 108.5 0.086 DOCOBO 20311+3333 17.6350 0.201 76.0 307.2 2008.5460 121.7 0.119 & CAMPO (*) SCARDIA, PRIEUR, PANSECCHI, LING, ARGYLE, ARISTIDI, ZANUTTA, ABE, BENDJOYA, RIVET, SUAREZ & VERNET 1 SARAH LEE LIPPINCOTT (1920-2019) Sarah Lee Lippincott was born in Philadelphia in 1920 and attended the University of Pennsylvania College for Women. -
A Bibliography of Publications in Computer Graphics World
A Bibliography of Publications in Computer Graphics World Nelson H. F. Beebe University of Utah Department of Mathematics, 110 LCB 155 S 1400 E RM 233 Salt Lake City, UT 84112-0090 USA Tel: +1 801 581 5254 FAX: +1 801 581 4148 E-mail: [email protected], [email protected], [email protected] (Internet) WWW URL: http://www.math.utah.edu/~beebe/ 21 June 2011 Version 1.18 Title word cross-reference 76 [Ano91b]. '90s [Rob93g]. '92 [Ano92-38]. '95 [Doy95]. '96 [Ano95-60]. 97 [Ano97-45]. 97/ FastSOLID [Ano97-37]. 98 [Ano98-47]. 1- [Tuc96]. 1.1 [Ano98-48]. 16-bit [Ano95-28]. A-h-h-h-h [Rob98h]. A/V [Har96a]. ABC [Spr94]. ABCs [Emm91c]. 2.0 [Gra96]. 21-inch [Ano95-29]. ability [Rob94a]. able [Coh96]. 2D [Coc95f, Mac90a]. 2nd [Ano96n]. Accelerating [Sch95a, Sch95b]. acceleration [Rob96d]. accelerator [Cla96]. 3.0 [Ano97-40]. 3.1 [Ano98-49]. accelerators [Coc95a, Ano95-34]. 3.5 [Ano97-44]. 3000 [Ano91-32]. acceptance [Rob94a]. 3D [Ano95-48, Coc95b, Ano90f, Rob90f]. accommodate [Pot97a]. 3D. [Ano98q]. 3D/Eye [Ano95-38]. According [Mah95c]. achieve [Emm94]. Achieving [Pot96a]. ACIS [Por95b]. 4.1 [Ano97-47]. 4.5 [Ano98-45]. Across [Sor90a]. Act [Rob94a]. 4D [Ano97-37]. Action [Mor93]. action-adventure [Rob96c]. 5 [Ano97-57]. 5.0 [Ano96-53]. 1 2 activity [RR97]. actual [Phi96e]. Photo [Ano90f]. Animation/ ADAMS [Ano95-52]. ADAMS/ Photo-Realism [Ano90f]. [Ano95-52]. Adding [Ano98q]. animations [Ano95-60, Phi95e]. addresses [Ano96-69]. Adds [Ano90n]. animator [Mah95c, Ano96-28]. adept [Pot96d]. adhered [Phi95e]. animators [Cra94]. Anime [Sav98]. Adobe [Ano96-50]. advance [Phi97e]. announced [Pot96e]. -
Exoplanet Meteorology: Characterizing the Atmospheres Of
Exoplanet Meteorology: Characterizing the Atmospheres of Directly Imaged Sub-Stellar Objects by Abhijith Rajan A Dissertation Presented in Partial Fulfillment of the Requirements for the Degree Doctor of Philosophy Approved April 2017 by the Graduate Supervisory Committee: Jennifer Patience, Co-Chair Patrick Young, Co-Chair Paul Scowen Nathaniel Butler Evgenya Shkolnik ARIZONA STATE UNIVERSITY May 2017 ©2017 Abhijith Rajan All Rights Reserved ABSTRACT The field of exoplanet science has matured over the past two decades with over 3500 confirmed exoplanets. However, many fundamental questions regarding the composition, and formation mechanism remain unanswered. Atmospheres are a window into the properties of a planet, and spectroscopic studies can help resolve many of these questions. For the first part of my dissertation, I participated in two studies of the atmospheres of brown dwarfs to search for weather variations. To understand the evolution of weather on brown dwarfs we conducted a multi- epoch study monitoring four cool brown dwarfs to search for photometric variability. These cool brown dwarfs are predicted to have salt and sulfide clouds condensing in their upper atmosphere and we detected one high amplitude variable. Combining observations for all T5 and later brown dwarfs we note a possible correlation between variability and cloud opacity. For the second half of my thesis, I focused on characterizing the atmospheres of directly imaged exoplanets. In the first study Hubble Space Telescope data on HR8799, in wavelengths unobservable from the ground, provide constraints on the presence of clouds in the outer planets. Next, I present research done in collaboration with the Gemini Planet Imager Exoplanet Survey (GPIES) team including an exploration of the instrument contrast against environmental parameters, and an examination of the environment of the planet in the HD 106906 system. -
New College News Release New College, Sarasota, Florida Furman C
/-·· NEW COLLEGE NEWS RELEASE NEW COLLEGE, SARASOTA, FLORIDA FURMAN C. ARTHUR - INFORMATION FOR RELEASE: Sunday, March 1, 1964 Sarasota--New College will have as its eighth lecturer in the New Perspectives in Science series Thursday at 8:00 p.m., Dutch born Dr. Peter van de Kamp, Director of the Sproul Observatory, swarthmore College. Dr. van de Kamp, the second astronomer in the series, approaches his field from a new viewpoint for the lecture at College Hall. He said that his talk will be about astronomy as a liberal art, "and by its very nature, peculiarly adapted to removing any artificial or imaginary bar- riers between the so-called sciences and the so-called liberal arts. Attendance at the lectures is by season registration although some single evening registrations are accepted. Born at Kampen in the Netherlands, Dr. van de Kamp was educated at the University of Utrecht where he studied astronomy, mathematics, and physics. Later, he obtained doctoral degrees at the University of California and the University of Groningen. Shortly after completing his education in the Netherlands, he came to this country to work at the McCormick Observatory at the University of Virginia and at the Lick Observatory at the University of California. (more) - 2 - Since 1937 he has been Director of the Sproul Observatory and Chairman of its Department of Astronomy. The Swarthmore observatory has one of the largest astronomical instruments of its kind. Dr. van de Kamp has taught or lectured a ·t many colleges in several countries. He is a former Fulbright scholar in France. During his education he was a member of Phi Beta Kappa and Sigma :· ~, honorary science research organization. -
Narrowband CCD Photometry of Giant HII Regions
Mon. Not. R. Astron. Soc. 000, 000–000 (0000) Printed 1 November 2018 (MN LATEX style file v2.2) Narrowband CCD Photometry of Giant HII Regions Guillermo Bosch 1 ⋆, Elena Terlevich 2 †, Roberto Terlevich 1 ‡ 1 Institute of Astronomy, Madingley Road, Cambridge CB3 0HA 2 INAOE, Puebla, M´exico 1 November 2018 ABSTRACT We have obtained accurate CCD narrow band Hβ and Hα photometry of Giant HII Regions in M 33, NGC 6822 and M 101. Comparison with previous determinations of emission line fluxes show large discrepancies; their probable origins are discussed. Combining our new photometric data with global velocity dispersion (σ) derived from emission line widths we have reviewed the L(Hβ)) − σ relation. A reanalysis of the properties of the GEHRs included in our sample shows that age spread and the su- perposition of components in multiple regions introduce a considerable spread in the regression. Combining the information available in the literature regarding ages of the associated clusters, evolutionary footprints on the interstellar medium, and kinemati- cal properties of the knots that build up the multiple GEHRs, we have found that a subsample - which we refer to as young and single GEHRs - do follow a tight relation in the L − σ plane. Key words: galaxies: individual: NGC6822, M33, M101 – H ii regions – galaxies: star clusters 1 INTRODUCTION tional explanation for this observed kinematical behaviour. Other authors confirmed the existence of a correlation, al- Accurate photometry of Giant HII Regions (GEHRs) is a though they found different slopes for the linear regression. key source of information about the energetics of these large New models were produced to account for the underlying dy- star-forming regions.