Why the Haiti Quake Killed So Many 3 Alive and Well 5 ESA Satellite
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
List of Reported UFO Sightings
List of reported UFO sightings This is a partial list by date of sightings of alleged unidentified flying objects (UFOs), including reports of close encounters and abductions. Contents Second millennium BCE Classical antiquity 16th–17th centuries 19th century 20th century 1901–1949 1950–1974 1975–2000 21st century By location See also Notes and references Second millennium BCE City, Date Name Country Description Sources State According to the disputed Tulli Papyrus, the scribes of the pharaoh Fiery Lower Ancient Thutmose III reported that "fiery disks" were encountered floating over ca. 1440 BCE [2][3] disks Egypt Egypt the skies. The Condon Committee disputed the legitimacy of the Tulli Papyrus stating, "Tulli was taken in and that the papyrus is a fake."[1] Classical antiquity City, Date Name Country Description Sources State Livy's Ab Livy records a number of portents in the winter of this year, including ships in Rome, Roman Urbe 218 BCE navium speciem de caelo adfulsisse ("phantom ships had been seen the sky Italia Republic Condita gleaming in the sky"). Libri[4][5] spark According to Pliny the Elder, a spark fell from a star and grew as it from a Roman 76 BCE unknown descended until it appeared to be the size of the Moon. It then ascended [6][5] falling Republic back up to the heavens and was transformed into a light. star According to Plutarch, a Roman army commanded by Lucullus was about flame- to begin a battle with Mithridates VI of Pontus when "all on a sudden, the like Phrygia, Roman sky burst asunder, and a huge, flame-like body was seen to fall between 74 BCE pithoi [7][5] Asia Republic the two armies. -
Mass Deficits, Stalling Radii, and the Merger Histories of Elliptical Galaxies David Merritt Rochester Institute of Technology
Rochester Institute of Technology RIT Scholar Works Articles 5-22-2006 Mass Deficits, Stalling Radii, and the Merger Histories of Elliptical Galaxies David Merritt Rochester Institute of Technology Follow this and additional works at: http://scholarworks.rit.edu/article Recommended Citation David Merritt 2006 ApJ 648 976 This Article is brought to you for free and open access by RIT Scholar Works. It has been accepted for inclusion in Articles by an authorized administrator of RIT Scholar Works. For more information, please contact [email protected]. DRAFT VERSION FEBRUARY 5, 2008 Preprint typeset using LATEX style emulateapj v. 10/09/06 MASS DEFICITS, STALLING RADII, AND THE MERGER HISTORIES OF ELLIPTICAL GALAXIES DAVID MERRITT Department of Physics, Rochester Institute of Technology, Rochester, NY 14623 Draft version February 5, 2008 Abstract A binary supermassive black hole leaves an imprint on a galactic nucleus in the form of a “mass deficit,” a decrease in the mass of the nucleus due to ejection of stars by the binary. The magnitude of the mass deficit is in principle related to the galaxy’s merger history, but the relation has never been quantified. Here, high- accuracy N-body simulations are used to calibrate this relation. Mass deficits are shown to be Mde f ≈ 0.5M12, with M12 the total mass of the binary; the coefficient in this relation depends only weakly on M2/M1 or on the galaxy’s pre-existing density profile. Hence, after N mergers, Mde f ≈ 0.5N M• with M• the final (current) black hole mass. When compared with observed mass deficits, this result implies 1 ∼< N ∼< 3, in accord with hierarchical galaxy formation models. -
Nonverbal Dictionary
The The NONVERBAL DICTIONARY of GESTURES, SIGNS & BODY LANGUAGE CUES From Adam's-Apple-Jump to Zygomatic Smile By David B. Givens © 2002 (Spokane, Washington: Center for Nonverbal Studies Press) Items in this Dictionary have been researched by anthropologists, archaeologists, biologists, linguists, psychiatrists, psychologists, semioticians, and others who have studied human communication from a scientific point of view. Every effort has been made to cite their work in the text. Definitions, meanings, and interpretations left uncredited are those of the author. Gestures and consumer products with http://members.aol.com/nonverbal2/diction1.htm (1 of 2) [27/04/02 05:54:42] The current trademark registrations are identified with the ® symbol. Entries in The Dictionary. There have been many who, not knowing how to mingle the useful and the pleasing in the right proportions, have had all their toil and pains for nothing . --Cervantes (Don Quixote) Dedication "A masterful piece of work" --American Library Association "Highly recommended" --New Scientist "Very interesting reading" --The Houston Chronicle "Monumental" --Yahoo! Picks of the Week "Site of the Day Award" --WWW Virtual Library WWW Virtual Library "Best" Site © 2002 by David B. Givens, Ph.D. Center for Nonverbal Studies http://members.aol.com/nonverbal2/diction1.htm (2 of 2) [27/04/02 05:54:42] adajum ADAM'S-APPLE-JUMP Body movement. 1. A conspicuous up-and-down motion of the Adam's apple. 2. A movement of the throat visible while gulping or swallowing, as in nervousness. Usage: The Adam's-apple-jump is an unconscious sign of emotional anxiety, embarrassment, or stress. -
Central Massive Objects: the Stellar Nuclei – Black Hole Connection
Astronomical News Report on the ESO Workshop Central Massive Objects: The Stellar Nuclei – Black Hole Connection held at ESO Garching, Germany, 22–25 June 2010 Nadine Neumayer1 Eric Emsellem1 1 ESO An overview of the ESO workshop on black holes and nuclear star clusters is presented. The meeting reviewed the status of our observational and the- oretical understanding of central mas- sive objects, as well as the search for intermediate mass black holes in globu- lar clusters. There will be no published proceedings, but presentations are available at http://www.eso.org/sci/ meetings/cmo2010/program.html. This workshop brought together a broad international audience in the combined fields of galaxy nuclei, nuclear star clus ters and supermassive black holes, to confront stateofthe art observations with cuttingedge models. Around a hundred participants from Europe, North and South America, as well as East Asia and Figure 1. Workshop participants assembled outside made up of several populations of stars. Australia gathered for a threeday meet ESO Headquarters in Garching. The existence of very young O and WR ing held at ESO Headquarters in Garching, stars in the central few arcseconds Germany (see Figure 1). The sessions around the black hole is puzzling. The were of very high quality, with many very – Are intermediate mass black holes currently favoured solution to this paradox lively, interesting and fruitful discussions. formed in nuclear clusters/globular of youth is in situ star formation in infalling All talks can be found online on the web clusters? gas clouds. This view is also supported page of the workshop1. -
Stellar Mass Function in the Field
Professor David Carter (PI) Liverpool John Moores University UK Dr Habib G. Khosroshahi Liverpool John Moores University UK Mr Mustapha Mouhcine Liverpool John Moores University UK Ms Susan M. Percival Liverpool John Moores University UK Dr Harry C. Ferguson (USA PI) Space Telescope Science Institute USA/MD Dr Paul Goudfrooij Space Telescope Science Institute USA/MD Dr Terry Bridges Queen's University Canada Dr Thomas H. Puzia Dominion Astrophysical Observatory Canada Dr Carlos del Burgo Dublin Institute For Advanced Studies Ireland Dr Bryan Miller Gemini Observatory, Southern Operations Chile Dr Bianca Poggianti INAF - Osservatorio Astronomico di Padova Italy Dr Alfonso Aguerri Instituto de Astrofisica de Canarias Spain Dr Marc Balcells Instituto de Astrofisica de Canarias Spain Mr Derek Hammer Johns Hopkins University USA/MD Dr Reynier F. Peletier Kapteyn Astronomical Institute Netherlands Prof. Edwin Valentijn Kapteyn Astronomical Institute Netherlands Dr Gijs Verdoes Kleijn Kapteyn Astronomical Institute Netherlands Dr Peter Erwin Max-Planck-Insitute for Extraterrestrial Physics Germany Dr Ann Hornschemeier NASA Goddard Space Flight Center USA/MD Dr Yutaka Komiyama National Astronomical Observatory of Japan Japan Dr Masafumi Yagi National Astronomical Observatory of Japan Japan Dr Jennifer Lotz National Optical Astronomy Observatories, AURA USA/AZ National Radio Astronomy Observatory, Dr Neal A. Miller USA/VA and Johns Hopkins University Dr Eric W. Peng Peking University China Dr Dan Batcheldor Rochester Institute of Technology USA/NY Prof. David Merritt Rochester Institute of Technology USA/NY Dr Ronald O. Marzke San Francisco State University USA/CA Dr Alister W. Graham Swinburne University of Technology Australia Dr Helmut Jerjen The Australian National University Australia Dr Avon P. -
Final 2013.Indd
SPECULATION ON ARCHITECTURE IN THE ABSENCE OF GRAVITY Speculation on Architecture in the absence of Gravity. How might architectural elements and design strategies function in outer space? Hermann Matamu 132 8392 Master Thesis explanatory document: Jeanette Budgett Abstract The evolution of architecture has been driven by a combination of elements such as style, context, materiality, aesthetic and technology. The development of materials and the technological advancements of the human race are conveyed through architecture; from the technical expertise of the ancient Egyptians in pyramid construction, to the engineering feats of the Eiffel Tower in Paris, to the physical realisation of Gehry’s Guggenheim through computer modelling. Architecture is a continuous evolution which revolves around the progression of the human race in all fields of life. Space habitation presents the next step in this architectural evolution, in which Space tourism acts as the stepping stone for the transition of architectural design beyond Earth. Space design has been produced largely without architectural input. The aim of this project is to introduce an architectural sensibility, and to investigate the impact an absence of gravitational force has on architecture. The research follows the transition of architectural design from an environment of gravity to one without, by reviewing both current literature and precedent case studies. i Acknowledgements As this chapter in my life comes to an end, I would like to thank all those who made it a memorable one. Firstly, I would like to thank my supervisor, Jeanette Budgett. Thank you for your patience, support and constant encouragement throughout my research, your knowledge and time have been instrumental in the development of this project. -
Accretion Onto a Quintessence Contaminated Rotating Black Hole : Violating the Lower Limit for Eta Over S Arxiv:1911.08304V2 [G
Accretion onto a Quintessence Contaminated Rotating Black Hole : Violating the Lower Limit for Eta over s Ritabrata Biswas 1 Promila Biswas 3 Parthajit Roy 2∗ 1;3 Department of Mathematics, The University of Burdwan Golapbag Academic Complex, City:Burdwan-713104, Dist: Purba Bardhaman, State: West Bengal, India 1e-mail: [email protected] 3e-mail: [email protected] 2Department of Computer Science, The University of Burdwan City:Burdwan-713104, Dist: Purba Bardhaman, State: West Bengal, India e-mail: [email protected] ∗ Abstract Viscous accretion flow around a rotating supermassive black hole sitting in a quintessence tub is studied in this article. To introduce such a dark energy contaminated black hole's gravitational force, a new pseudo-Newtonian potential is used. This pseudo-Newtonian force can be calculated if we know the distance from the black hole's center, spin of the black hole and equation of state of the quintessence inside which the black hole is considered to lie. This force helps us to avoid complicated nonlinearity of general relativistic field equations. Transonic, viscous, continuous and Keplerian flow is assumed to take place. Fluid speed, sonic speed profile and specific angular momentum to Keplerian angular momentum ratio are found out for different values of spin parameter and arXiv:1911.08304v2 [gr-qc] 2 Mar 2021 quintessence parameter. Density variation is built and tallied with observations. Shear viscosity to entropy density ratio is constructed for our model and a comparison with theoretical lower limit is done. Keywords: Accretion Disc, Viscosity, Quintessence, Supermassive Black Holes, Shear Viscosity to entropy ratio PACS: 97.10.Gz; 51.20.+d; 51.30.+i; 95.36.+x; 97.60.25 1 Introduction Since 1998, despite the propositions of different conceptual models, we were not really able to construct a hundred percent correct theoretical support to the observations of late time cosmic acceleration. -
The Star Clusters Young & Old Newsletter
SCYON The Star Clusters Young & Old Newsletter edited by Holger Baumgardt, Ernst Paunzen and Pavel Kroupa SCYON can be found at URL: http://astro.u-strasbg.fr/scyon SCYONIssueNo.31 11December2006 EDITORIAL Here is the 31st issue of the SCYON newsletter. The current issue contains 35 abstracts, an an- nouncement for a new, parallel N-body code and announcements for conferences in Italy, Germany and Armenia. It also contains job advertisements for postdoctoral and tenure track positions from Rochester Institute of Technology. We wish everybody a merry holiday season and a happy new year 2007 and thank those who sent us their contributions. Holger Baumgardt, Ernst Paunzen and Pavel Kroupa ................................................... ................................................. CONTENTS Editorial .......................................... ...............................................1 SCYON policy ........................................ ...........................................2 Mirror sites ........................................ ..............................................2 Abstract from/submitted to REFEREED JOURNALS ........... ................................3 1. Star Forming Regions ............................... ........................................3 2. Embedded Clusters................................. .........................................7 3. Galactic Center Clusters........................... ..........................................9 4. Galactic Open Clusters............................. ........................................10 -
Galactic Nuclei
Relativity, torque and spin PROFESSOR DAVID MERRITT DAVID PROFESSOR Professor David Merritt explains his interest in astrophysics and the focus of his current research. Describing the improvements made to the computational algorithms, he highlights the importance of taking into account the effects of relativity in these calculations sometimes reveal modes of behaviour that can be inefficient when applied to galactic are strikingly simple yet totally unexpected. nuclei, because motion is dominated by the presence of the SBH. A star or stellar remnant Your current project focuses on the dynamical will complete millions of orbits around evolution of dense clusters of stars and the SBH before coming close enough to stellar remnants around supermassive black another star to be perturbed, but it is those holes (SBHs) at the centre of galaxies. Why is perturbations that are driving the collective this important? evolution. The computer code needs to follow the unperturbed orbit about the SBH with A star like the Sun would be tidally torn apart extremely high precision: otherwise the effects if it came sufficiently close to an SBH. Partly of the small perturbations will be swamped by because of tidal effects, the only objects numerical errors. that we expect to find very near an SBH are ‘compact remnants’: neutron stars and Why is it important to take into account stellar-mass black holes, the dense leftovers the effects of relativity when simulating the from the evolution of massive stars. These evolution of nuclear star clusters? remnants can interact through ‘gravitational encounters’: close passages that exchange One insight that comes from my group’s research energy and gradually change orbits. -
Science Service
Rs. 275/- ISSN 0970-6488 Science Service www.ptinews.com Vol 37 No. 13 (20 pages including cover) CONTENTS NATIONAL SCIENCE BRIEFS: * New book delves into India’s nuclear doctrine evolution * Symposium on rise in drug resistant bacteria held at IMTECH * Nadda launches National Health Resource Repositry * Yoga helps reduce severity of depressiona AIIIMS study * Expert panel will be set up yo use advanced technology to deal with air pollution Env Ministry * Satya Pal Singh asks IIT-G to also work on ancient tecnologies * Use of diesel generators increased pollution levels in Gurgaon residential socities: CSE * Govt sets up panels under task force for implementing drone tech * Most people aware of harmful effects of plastics but still use it :study . INTERNATIONAL SCIENCE BRIEFS: * World ‘s smalleast computer device created * Novel keyboard can be crumpled ,carried in pockets * Printed sensors may turn gummy bears into ingestible medical probes * New ‘e- skin’ brings sense of touch to prosthetic hands *NASA’s curiosity rover captures photos of Mars dust storm * Faster, cheaper way to synthesis DNA developed * Smart stents can better prevent heart attacks *New system lets you control robots with brain waves, hand gestures * China to set up varisty for nuclear power research * Evidence of rare black hole spotted * Space tourists may not be prepared for trip beyond earth:NASA astronaut * Last of universe, smissing ordinary matter found * NASA delays James webb Space Telescope launch to 2021 * Don’t be over the moon yet! Buying a piece of lunar landscape still a distant dream * Milky way full of ‘space grease’: Study * Organic molecules on saturn’s moon indicate possibility of life * Sweden, Finland developing technology to curb India’s pollution woes * Scientist develop ”deep learning” robots to empower autistic children * SpaceX launches AI robot, strong coffee for station crew. -
Extracting the Gravitational Recoil from Black Hole Merger Signals
Extracting the Gravitational Recoil from Black Hole Merger Signals Vijay Varma,1, ∗ Maximiliano Isi,2, † and Sylvia Biscoveanu2, ‡ 1TAPIR 350-17, California Institute of Technology, 1200 E California Boulevard, Pasadena, CA 91125, USA 2LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA (Dated: March 11, 2020) Gravitational waves carry energy, angular momentum, and linear momentum. In generic binary black hole mergers, the loss of linear momentum imparts a recoil velocity, or a “kick”, to the remnant black hole. We exploit recent advances in gravitational waveform and remnant black hole modeling to extract information about the kick from the gravitational wave signal. Kick measurements such as these are astrophysically valuable, enabling independent constraints on the rate of second-generation mergers. Further, we show that kicks must be factored into future ringdown tests of general relativity with third-generation gravitational wave detectors to avoid systematic biases. We find that, although little information can be gained about the kick for existing gravitational wave events, interesting measurements will soon become possible as detectors improve. We show that, once LIGO and Virgo reach their design sensitivities, we will reliably extract the kick velocity for generically precessing binaries—including the so-called superkicks, reaching up to 5000 km/s. Introduction.— As existing gravitational wave (GW) de- galactic centers. The remnant BH can be significantly tectors, Advanced LIGO [1] and Virgo [2], approach their displaced or ejected [31, 32], impacting the galaxy’s evo- design sensitivities, they continue to open up unprece- lution [33–35], and event rates [36] for the future LISA dented avenues for studying the astrophysics of black mission [37]. -
Highlights in Space 2010
International Astronautical Federation Committee on Space Research International Institute of Space Law 94 bis, Avenue de Suffren c/o CNES 94 bis, Avenue de Suffren 75015 Paris, France 2 place Maurice Quentin 75015 Paris, France UNITED NATIONS Tel: +33 1 45 67 42 60 75039 Paris Cedex 01, France E-mail: : [email protected] Fax: +33 1 42 73 21 20 Tel. + 33 1 44 76 75 10 URL: www.iislweb.com E-mail: [email protected] Fax. + 33 1 44 76 74 37 OFFICE FOR OUTER SPACE AFFAIRS URL: www.iafastro.com E-mail: [email protected] URL: http://cosparhq.cnes.fr Highlights in Space 2010 Prepared in cooperation with the International Astronautical Federation, the Committee on Space Research and the International Institute of Space Law The United Nations Office for Outer Space Affairs is responsible for promoting international cooperation in the peaceful uses of outer space and assisting developing countries in using space science and technology. United Nations Office for Outer Space Affairs P. O. Box 500, 1400 Vienna, Austria Tel: (+43-1) 26060-4950 Fax: (+43-1) 26060-5830 E-mail: [email protected] URL: www.unoosa.org United Nations publication Printed in Austria USD 15 Sales No. E.11.I.3 ISBN 978-92-1-101236-1 ST/SPACE/57 V.11-80947—March*1180947* 2011—475 UNITED NATIONS OFFICE FOR OUTER SPACE AFFAIRS UNITED NATIONS OFFICE AT VIENNA Highlights in Space 2010 Prepared in cooperation with the International Astronautical Federation, the Committee on Space Research and the International Institute of Space Law Progress in space science, technology and applications, international cooperation and space law UNITED NATIONS New York, 2011 UniTEd NationS PUblication Sales no.