The Messenger
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
FY08 Technical Papers by GSMTPO Staff
AURA/NOAO ANNUAL REPORT FY 2008 Submitted to the National Science Foundation July 23, 2008 Revised as Complete and Submitted December 23, 2008 NGC 660, ~13 Mpc from the Earth, is a peculiar, polar ring galaxy that resulted from two galaxies colliding. It consists of a nearly edge-on disk and a strongly warped outer disk. Image Credit: T.A. Rector/University of Alaska, Anchorage NATIONAL OPTICAL ASTRONOMY OBSERVATORY NOAO ANNUAL REPORT FY 2008 Submitted to the National Science Foundation December 23, 2008 TABLE OF CONTENTS EXECUTIVE SUMMARY ............................................................................................................................. 1 1 SCIENTIFIC ACTIVITIES AND FINDINGS ..................................................................................... 2 1.1 Cerro Tololo Inter-American Observatory...................................................................................... 2 The Once and Future Supernova η Carinae...................................................................................................... 2 A Stellar Merger and a Missing White Dwarf.................................................................................................. 3 Imaging the COSMOS...................................................................................................................................... 3 The Hubble Constant from a Gravitational Lens.............................................................................................. 4 A New Dwarf Nova in the Period Gap............................................................................................................ -
EXTENSIONS of REMARKS November 19, 1975 We Can Save a Great Deal in Those the Budget Committee, the Senior Sena
37480 EXTENSIONS OF REMARKS November 19, 1975 We can save a great deal in those the Budget Committee, the senior Sena . Upon the disposition of the congres amounts. But with such things as social tor from Maine (Mr. MusKIE) and the sional budget resolution, the Senate will security, retirement programs, and pen distinguished ranking minority member take up the Interior appropriation bill, sions, we are not going to reduce those, of the committee, the senior Senator with a rollcall vote expected on final and I think we all recognize that. from Oklahoma (Mr. BELLMON). passage. Mr. DOMENICI. There may be some In the past year they have assembled The Senate conceivably could be in reform necessary, and that might occur, a truly excellent staff, and proved that session until a reasonably late hour to but I think my distinguished chairman is the complex provisions of the budget and morrow, with rollcall votes throughout. saying if the Budget Committee were to Impoundment Control Act of 1974 can put a figure in other than the real outlay in fact help to reassert the congressional expected for one of those programs we control over the Nation's purse that the RECESS UNTIL 8:45 A.M. would be fooling ourselves and we would Constitution provides. Mr. MUSKIE. Mr. President, if there be fooling the American people on the Over the past year I have often dis is nothing further that any Senator budget, because there is a legal entitle agreed with a majority of the committee wishes to say at this time, I move that ment that exists in the field on the part on specific issues. -
Dark Matter and Dark Energy
HTS Teologiese Studies/Theological Studies ISSN: (Online) 2072-8050, (Print) 0259-9422 Page 1 of 8 Original Research The building blocks of the universe Author: I review the state of knowledge of the composition of the universe for a non-specialist audience. 1,2 Anslyn J. John The universe is built up of four components. These are radiation, baryonic (ordinary) matter, Affiliation: dark matter and dark energy. In this article, a quick outline of the theory of Big Bang 1Department of Physics, nucleosynthesis is presented, and the origin of the elements is explained. Cosmology requires Faculty of Science, the presence of dark matter, which forms most of the mass of the universe, and dark energy, Stellenbosch University, which drives the acceleration of the expansion. The dark sector is motivated, and possible Stellenbosch, South Africa explanations are stated. 2National Institute for Contribution: As part of this special collection on building blocks, the building blocks of the Theoretical and Computational Sciences universe are discussed and unsolved problems and proposed solutions are highlighted. (NITheCS), South Africa Keywords: cosmology; nucleosynthesis; dark matter; dark energy; cosmological constant; Corresponding author: general relativity; galaxies; particle physics. Anslyn John, [email protected] Dates: Introduction Received: 10 May 2021 Cosmology is the scientific study of the origin and development of the universe on the largest Accepted: 12 July 2021 Published: 25 Aug. 2021 scales. Today, the standard model of cosmology is a cornerstone of physics and astronomy. This is attested to by the award of four Nobel Prizes for research in cosmology. These awards, in How to cite this article: chronological order, are: John, A.J., 2021, ‘The building blocks of the universe’, 1. -
NENHC 2008 Abstracts
Abstracts APRIL 17 – APRIL 18, 2008 A FORUM FOR CURRENT RESEARCH The Northeastern Naturalist The New York State Museum is a program of The University of the State of New York/The State Education Department APRIL 17 – APRIL 18, 2008 A FORUM FOR CURRENT RESEARCH SUGGESTED FORMAT FOR CITING ABSTRACTS: Abstracts Northeast Natural History Conference X. N.Y. State Mus. Circ. 71: page number(s). 2008. ISBN: 1-55557-246-4 The University of the State of New York THE STATE EDUCATION DEPARTMENT ALBANY, NY 12230 THE UNIVERSITY OF THE STATE OF NEW YORK Regents of The University ROBERT M. BENNETT, Chancellor, B.A., M.S. ................................................................. Tonawanda MERRYL H. TISCH, Vice Chancellor, B.A., M.A., Ed.D. ................................................. New York SAUL B. COHEN, B.A., M.A., Ph.D.................................................................................. New Rochelle JAMES C. DAWSON, A.A., B.A., M.S., Ph.D. .................................................................. Peru ANTHONY S. BOTTAR, B.A., J.D. ..................................................................................... Syracuse GERALDINE D. CHAPEY, B.A., M.A., Ed.D. ................................................................... Belle Harbor ARNOLD B. GARDNER, B.A., LL.B. .................................................................................. Buffalo HARRY PHILLIPS, 3rd, B.A., M.S.F.S. ............................................................................. Hartsdale JOSEPH E. BOWMAN, JR., B.A., -
Prof. Mustafa Türker ÖZKAN
Prof. Mustafa Türker ÖZKAN OPfefricseo Pnhaol nIen:f +or9m0 2a1t2io 4n40 0369 Extension: 10294 EFmaxa iPl:h oznkea:n +t@9i0s t2a1n2b u4l4.e0d u0.3tr70 AWdedbr:e hstst:p :A/s/tarvoenso.imstia vneb uUlz.eadyu B.tirli/molzekrai nBtö/lümü, İstanbul Üniversitesi Beyazıt Yerleşkesi, 34119, Fatih-İstanbul EDodcutocraatteio, İnst aInnbfuol rÜmniavetriosintesi, Faculty of Science, Astronomi Ve Uzay Bilimleri, Turkey 1981 - 1987 UPonsdtegrrgardaudautaet, eİs, tİastnabnublu Ül nÜinveivresritseitsei,s Fi, aFcauclutylt oy fo Sfc Siecniecnec, eA, sAtrsotrnoonmomi Vi eV Ue zUazya By iBlimilimlerlei,r Ti, uTrukrekye 1y 917987 3- 1- 9189077 FEnogrliesihg, nB2 L Uapnpgeru Iangteersmediate Dissertations ADsotcrtoonroamtey, G aünnde Sşp Laeckee Slecrieinndceks,i 1D9o8ğ7u-Batı Asimetrisinin Nedenleri Üzerine, Istanbul University, Faculty of Science, APostsrtognraodmuya taen, dP lSapnaect ev eS cÇieifnt-cYeısld, 1ız9 Y8ö0rüngelerinde Büyük Eksen Dönmesi, Istanbul University, Faculty of Science, Research Areas aPnhdy sOicbss, eArsvtartoionnosm, yS taanrsd, ANsattruorpahl ySsciicesn, cSeusn and Solar Systems, Astronomy and Astrophysics: Instrumentation Techniques Academic Titles / Tasks APrsosofecsiastoer ,P Irsotafensbsuolr U, Insitvaenrbsuitly U, Fnaivceurltsyit yo,f FSaccieunltcye o, Af sStcrioencoem, Ay satnrodn Sopmacye a Sncdie Snpcaecse, 1S9c9ie5n c- eCso, n1t9in9u0e -s 1995 RAessiesatarcnht PArsosfisetsasnotr, ,İ Issttaannbbuul lÜ Unniviveerrssititeys,i ,F Faaccuultlyty o of fS Sccieiennccee, ,A Asstrtroonnoommyy a anndd S Sppaaccee S Sccieienncceess, -
Booklet 2008-09.Indd
The Shaw Prize The Shaw Prize is an international award to honour individuals who are currently active in their respective fields and who have achieved distinguished and significant advances, who have made outstanding contributions in culture and the arts, or who in other domains have achieved excellence. The award is dedicated to furthering societal progress, enhancing quality of life, and enriching humanity’s spiritual civilization. Preference will be given to individuals whose significant work was recently achieved. Founder's Biographical Note The Shaw Prize was established under the auspices of Mr Run Run Shaw. Mr Shaw, born in China in 1907, is a native of Ningbo County, Zhejiang Province. He joined his brother’s film company in China in the 1920s. In the 1950s he founded the film company Shaw Brothers (Hong Kong) Limited in Hong Kong. He has been Executive Chairman of Television Broadcasts Limited in Hong Kong since the 1970s. Mr Shaw has also founded two charities, The Sir Run Run Shaw Charitable Trust and The Shaw Foundation Hong Kong, both dedicated to the promotion of education, scientific and technological research, medical and welfare services, and culture and the arts. ~ 1 ~ Message from the Chief Executive I am delighted to congratulate the six distinguished scientists who receive this year’s Shaw Prize. Their accomplishments enrich human knowledge and have a profound impact on the advancement of science. This year, the Shaw Prize recognises remarkable achievements in the areas of astronomy, life science and medicine, and mathematical sciences. The exemplary work and dedication of this year’s recipients vividly demonstrate that constant drive for excellence will eventually bear fruit. -
A Photometric Study of Be Stars Located in the Seismology fields of COROT
A&A 476, 927–933 (2007) Astronomy DOI: 10.1051/0004-6361:20078252 & c ESO 2007 Astrophysics A photometric study of Be stars located in the seismology fields of COROT J. Gutiérrez-Soto1,2,J.Fabregat1,2,J.Suso3, M. Lanzara3, R. Garrido4, A.-M. Hubert2, and M. Floquet2 1 Observatorio Astronómico, Universidad de Valencia, edificio Institutos de Investigación, polígono la Coma, 46980 Paterna, Valencia, Spain e-mail: [email protected] 2 GEPI, Observatoire de Paris, CNRS, Université Paris Diderot; place Jules Janssen 92195 Meudon Cedex, France 3 GACE-ICMUV, edificio Institutos de Investigación, polígono la Coma, 46980 Paterna, Valencia, Spain 4 Instituto de Astrofísica de Andalucía (CSIC), calle Camino Bajo de Huétor, 24. 18008, Granada, Spain Received 10 July 2007 / Accepted 28 September 2007 ABSTRACT Context. In preparation for the COROT mission, an exhaustive photometric study of Be stars located in the seismology fields of the mission has been performed. The very precise and long-time-spanned photometric observations gathered by the COROT satellite will give important clues on the origin of the Be phenomenon. Aims. The aim of this work is to find short-period variable Be stars located in the seismology fields of COROT, and to study and characterise their pulsational properties. Methods. Light curves obtained at the Observatorio de Sierra Nevada, together with data from Hipparcos and ASAS-3 for a total of 84 Be stars, were analysed in order to search for short-term variations. We applied standard Fourier techniques and non-linear least-square fitting to the time series. Results. We found 7 multiperiodic, 21 mono-periodic and 26 non-variable Be stars. -
Measuring the Stellar Accretion Rates of Herbig Ae/Be Stars Brian Donehew Clemson University
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by Clemson University: TigerPrints Clemson University TigerPrints Publications Physics and Astronomy 1-1-2012 Measuring the Stellar Accretion Rates of Herbig Ae/Be Stars Brian Donehew Clemson University Sean D. Brittain Clemson University, [email protected] Follow this and additional works at: https://tigerprints.clemson.edu/physastro_pubs Part of the Astrophysics and Astronomy Commons Recommended Citation Please use publisher's recommended citation. This Article is brought to you for free and open access by the Physics and Astronomy at TigerPrints. It has been accepted for inclusion in Publications by an authorized administrator of TigerPrints. For more information, please contact [email protected]. The Astronomical Journal, 141:46 (10pp), 2011 February doi:10.1088/0004-6256/141/2/46 C 2011. The American Astronomical Society. All rights reserved. Printed in the U.S.A. MEASURING THE STELLAR ACCRETION RATES OF HERBIG Ae/Be STARS Brian Donehew1 and Sean Brittain1 Department of Physics and Astronomy, Clemson University, Clemson, SC 29634-0978, USA; [email protected], [email protected] Received 2010 April 10; accepted 2010 November 10; published 2011 January 12 ABSTRACT The accretion rate of young stars is a fundamental characteristic of these systems. While accretion onto T Tauri stars has been studied extensively, little work has been done on measuring the accretion rate of their intermediate-mass analogs, the Herbig Ae/Be stars. Measuring the stellar accretion rate of Herbig Ae/Bes is not straightforward both because of the dearth of metal absorption lines available for veiling measurements and the intrinsic brightness of Herbig Ae/Be stars at ultraviolet wavelengths where the brightness of the accretion shock peaks. -
Asia Pacific Physics Newsletter
Asia Pacific Physics Newsletter March 2016 Volume 5 • Number 1 worldscinet.com/appn Takaaki Kajita 2015 Physics Nobel Laureate published by Institute of Advanced Studies, Nanyang Technological University (IAS@NTU) and South East Asia Theoretical Physics Association (SEATPA) South East Asia Theoretical Physics Association Asia Pacific Physics Newsletter March 2016 • Volume 5 • Number 1 A publication of the IAS@NTU Singapore and SEATPA Asia Pacific Physics Newsletter publishes articles reporting frontier discoveries in EDITORIAL physics, research highlights, and news to facilitate interaction, collaboration and 3 cooperation among physicists in Asia Pacific physics community. PEOPLE Editor-in-Chief 4 “Observing the Distant Supernova” — Interview with Kok Khoo Phua Nobel Laureate Prof Brian Schmidt Associate Editor-in-Chief “Discovering the W and Z Bosons” — Interview with Swee Cheng Lim Nobel Laureate Prof Carlo Rubbia SEATPA Committee Christopher C Bernido Phil Chan Leong Chuan Kwek Choy Heng Lai Swee Cheng Lim Ren Bao Liu Hwee Boon Low Anh Ký Nguyên Choo Hiap Oh OPINION AND COMMENTARY Kok Khoo Phua 10 China’s Great Scientific Leap Forward: Completion of a Roh Suan Tung Preecha Yupapin planned ‘Great Collider’ would transform particle physics Hishamuddin Zainuddin Freddy Zen Editorial Team NEWS Sen Mu 12 CityU’s Institute for Advanced Study will Champion Bold New Han Sun Chi Xiong Research Initiatives Case made for 'Ninth Planet' Graphic Designers Chuan Ming Loo Erin Ong Cover Photo: "Takaaki Kajita 5171- 2015" by Bengt Nyman - Own work. -
Structure of Herbig Aebe Disks at the Milliarcsecond Scale a Statistical Survey in the H Band Using PIONIER-VLTI? B
A&A 599, A85 (2017) Astronomy DOI: 10.1051/0004-6361/201629305 & c ESO 2017 Astrophysics Structure of Herbig AeBe disks at the milliarcsecond scale A statistical survey in the H band using PIONIER-VLTI? B. Lazareff1, J.-P. Berger2,1, J. Kluska3, J.-B. Le Bouquin1, M. Benisty1, F. Malbet1, C. Koen4, C. Pinte6,20, W.-F. Thi7, O. Absil5,??, F. Baron8, A. Delboulbé1, G. Duvert1, A. Isella10, L. Jocou1, A. Juhasz9, S. Kraus3, R. Lachaume11,12, F. Ménard1, R. Millan-Gabet14,15, J. D. Monnier13, T. Moulin1, K. Perraut1, S. Rochat1, F. Soulez16,17, M. Tallon16, E. Thiébaut16, W. Traub18, and G. Zins19 1 Univ. Grenoble Alpes, IPAG; CNRS, IPAG, 38000 Grenoble, France e-mail: [email protected] 2 ESO, Karl-Schwarzschild-Strasse 2, 85748 Garching bei München, Germany 3 University of Exeter, Department of Physics and Astronomy, Stocker Road, Exeter, Devon EX4 4QL, UK 4 Department of Statistics, University of the Western Cape, Private Bag X17, 7535 Bellville, South Africa 5 STAR, Université de Liège, 19c allée du Six Août, 4000 Liège, Belgium 6 UMI-FCA, CNRS/INSU, France 7 Max-Planck-Institut für Extraterrestrische Physik, 85748 Garching, Germany 8 Center for High Angular Resolution Astronomy, Georgia State University, PO Box 3969, Atlanta, GA 30302, USA 9 Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge, CB3 0HA, UK 10 Department of Physics and Astronomy, Rice University, 6100 Main Street, Houston, TX 77005, USA 11 Centro de Astroingeniería, Instituto de Astrofísica, Facultad de Física, Pontificia Universidad Católica de Chile, Casilla 306, Santiago 22, Chile 12 Max-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany 13 Department of Astronomy, University of Michigan, 1085 S. -
Science & ROGER PENROSE
Science & ROGER PENROSE Live Webinar - hosted by the Center for Consciousness Studies August 3 – 6, 2021 9:00 am – 12:30 pm (MST-Arizona) each day 4 Online Live Sessions DAY 1 Tuesday August 3, 2021 9:00 am to 12:30 pm MST-Arizona Overview / Black Holes SIR ROGER PENROSE (Nobel Laureate) Oxford University, UK Tuesday August 3, 2021 9:00 am – 10:30 am MST-Arizona Roger Penrose was born, August 8, 1931 in Colchester Essex UK. He earned a 1st class mathematics degree at University College London; a PhD at Cambridge UK, and became assistant lecturer, Bedford College London, Research Fellow St John’s College, Cambridge (now Honorary Fellow), a post-doc at King’s College London, NATO Fellow at Princeton, Syracuse, and Cornell Universities, USA. He also served a 1-year appointment at University of Texas, became a Reader then full Professor at Birkbeck College, London, and Rouse Ball Professor of Mathematics, Oxford University (during which he served several 1/2-year periods as Mathematics Professor at Rice University, Houston, Texas). He is now Emeritus Rouse Ball Professor, Fellow, Wadham College, Oxford (now Emeritus Fellow). He has received many awards and honorary degrees, including knighthood, Fellow of the Royal Society and of the US National Academy of Sciences, the De Morgan Medal of London Mathematical Society, the Copley Medal of the Royal Society, the Wolf Prize in mathematics (shared with Stephen Hawking), the Pomeranchuk Prize (Moscow), and one half of the 2020 Nobel Prize in Physics, the other half shared by Reinhard Genzel and Andrea Ghez. -
RS Puppis | AAVSO 2/7/11 12:45 PM
RS Puppis | AAVSO 2/7/11 12:45 PM Search About Us Community Variable Stars Observing Data Education & Outreach 100 Years of Citizen Astronomy 1911-2011 Home Contact Us FAQ Donate Home RS Puppis RS Puppis as imaged with the ESO NTT (from Kervella et al. 2008) January is a good time of year to observe this month's Variable Star of the Season, RS Puppis. A bright, southern gem, RS Pup has been known since the end of the 19th century, and has provided variable star observers and researchers with a bright and interesting target throughout its history. RS Pup is a delta Cephei star, or Cepheid Variable, a Milky Way member of this cosmically important class of stars that let us measure distances in the universe. However, RS Pup is in a class of its own as a star that produces light echoes of its pulsations visible in the nebula that surrounds it. This month, join us as we learn a little more about this lovely southern target of our January skies. Discovery One of the earliest mentions of RS Pup in the literature was in a short report by David Gill, then director of Cape Observatory, that appeared in Astronomisches Nachrichten in 1897. Gill was himself passing along the observations of the noted visual observer R.T.A. Innes, a largely self-taught Scotsman who rose to become one of the preeminent observers of the southern hemisphere, and eventual director of the Transvaal Meteorological Department (Republic Observatory at Johannesburg). In his half-page report on suspected variables of J.C.