Portland Daily Press: December 22, 1896
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Lurking in the Shadows: Wide-Separation Gas Giants As Tracers of Planet Formation
Lurking in the Shadows: Wide-Separation Gas Giants as Tracers of Planet Formation Thesis by Marta Levesque Bryan In Partial Fulfillment of the Requirements for the Degree of Doctor of Philosophy CALIFORNIA INSTITUTE OF TECHNOLOGY Pasadena, California 2018 Defended May 1, 2018 ii © 2018 Marta Levesque Bryan ORCID: [0000-0002-6076-5967] All rights reserved iii ACKNOWLEDGEMENTS First and foremost I would like to thank Heather Knutson, who I had the great privilege of working with as my thesis advisor. Her encouragement, guidance, and perspective helped me navigate many a challenging problem, and my conversations with her were a consistent source of positivity and learning throughout my time at Caltech. I leave graduate school a better scientist and person for having her as a role model. Heather fostered a wonderfully positive and supportive environment for her students, giving us the space to explore and grow - I could not have asked for a better advisor or research experience. I would also like to thank Konstantin Batygin for enthusiastic and illuminating discussions that always left me more excited to explore the result at hand. Thank you as well to Dimitri Mawet for providing both expertise and contagious optimism for some of my latest direct imaging endeavors. Thank you to the rest of my thesis committee, namely Geoff Blake, Evan Kirby, and Chuck Steidel for their support, helpful conversations, and insightful questions. I am grateful to have had the opportunity to collaborate with Brendan Bowler. His talk at Caltech my second year of graduate school introduced me to an unexpected population of massive wide-separation planetary-mass companions, and lead to a long-running collaboration from which several of my thesis projects were born. -
Sanelli Colore
CATALOGO GENERALE CARATTERISTICHE Lame SKIN Acciaio inox Bonpertuis specifico per coltelleria. PRINCIPALI Elevata durezza (54-56 HRC). MAIN FEATURES Ottima flessibilità. Elevato potere tranciante. CARACTÉRISTIQUES Filo a profilo convesso, controllato artigianalmente. PRINCIPALES Particolarmente studiato per uso professionale, garanzia di lunga durata. SKIN Blades Bonpertuis stainless steel specific for cutlery. High hardness (54-56 HRC). Excellent flexibility. High cutting power. Convex cutting-edge, hand-checked. Particularly designed for professional use, long life guarantee. Lames SKIN Acier inoxydable Bonpertuis spécifique pour coutellerie. Fermeté résistente (54-56 HRC). Bonne flexibilité Un potentiel tranchant élevé. Forme convexe du fil, à la main. Spécialement conçu pour un usage professionnel, garantie de longue durée. Manici SKIN Innovativa mescola di polipropilene. Design ergonomico esclusivo. Texturizzazione superficie a rugosità calibrata per una presa sicura. SKIN Handles New mix of polypropylene. Exclusive ergonomic design. Surface texturization with calibrated roughness for a safe grip. Manches SKIN Nouveau mélange de polypropylène. Design ergonomique exclusif. Texturation de la surface avec rugosité calibrée pour une prise sûre. MADE IN ITALY 39 348324 Mezzaluna manico tondo Mincing knife round handle Hachoir poignée ronde Lama/blade/lame 24 cm 348424 Mezzaluna manico piatto Mincing knife flat handle Hachoir poignée plate SKIN Lama/blade/lame 24 cm CARNI COTTE E POLLAME 100218.G Francese Butcher Boucher Lama/blade/lame -
Naming the Extrasolar Planets
Naming the extrasolar planets W. Lyra Max Planck Institute for Astronomy, K¨onigstuhl 17, 69177, Heidelberg, Germany [email protected] Abstract and OGLE-TR-182 b, which does not help educators convey the message that these planets are quite similar to Jupiter. Extrasolar planets are not named and are referred to only In stark contrast, the sentence“planet Apollo is a gas giant by their assigned scientific designation. The reason given like Jupiter” is heavily - yet invisibly - coated with Coper- by the IAU to not name the planets is that it is consid- nicanism. ered impractical as planets are expected to be common. I One reason given by the IAU for not considering naming advance some reasons as to why this logic is flawed, and sug- the extrasolar planets is that it is a task deemed impractical. gest names for the 403 extrasolar planet candidates known One source is quoted as having said “if planets are found to as of Oct 2009. The names follow a scheme of association occur very frequently in the Universe, a system of individual with the constellation that the host star pertains to, and names for planets might well rapidly be found equally im- therefore are mostly drawn from Roman-Greek mythology. practicable as it is for stars, as planet discoveries progress.” Other mythologies may also be used given that a suitable 1. This leads to a second argument. It is indeed impractical association is established. to name all stars. But some stars are named nonetheless. In fact, all other classes of astronomical bodies are named. -
CATALOGUE SUPPLÉMENTAIRE 2020 6438 Ibach-Schwyz, Suisse T + 41 41 81 81 211 F + 41 41 81 81 511 COUTEAUX SUISSES Info @ Victorinox.Com
Victorinox AG Schmiedgasse 57 CATALOGUE SUPPLÉMENTAIRE 2020 6438 Ibach-Schwyz, Suisse T + 41 41 81 81 211 F + 41 41 81 81 511 COUTEAUX SUISSES info @ victorinox.com Contact UE: Victorinox Retail Köln GmbH Wallrafplatz 2 50667 Köln, Allemagne VICTORINOX.COM Printed in Switzerland © Victorinox 2019 We protect our intellectual property rights. We reserve our rights for technical modifications. 128768 FROM THE MAKERS OF THE ORIGINAL SWISS ARMY KNIFE™ 611160 7 ESTABLISHED 1884 XII.19 / 9.2104.3 XII.19 / 9.2104.3 CATALOGUE SUPPLÉMENTAIRE 2020 COUTEAUX SUISSES 1 2 PETITS COUTEAUX DE POCHE SWISS TOOLS SPORT COUTEAUX DE POCHE, TAILLE MOYENNE MANICURE ET PÉDICURE GRANDS COUTEAUX DE POCHE ACCESSOIRES PETITS COUTEAUX DE POCHE SWISS TOOLS 05 Nail Clip 580 Set 37 Swiss Tool Spirit XBS 14 Classic SD Wood 37 Swiss Tool BS 21 Classic Navy Camouflage SPORT COUTEAUX DE POCHE, 41 Outdoor Master Mic S TAILLE MOYENNE 41 Outdoor Master Mic L 08 Spartan PS 11 Spartan Wood MANICURE ET PÉDICURE 11 Huntsman Wood 45 Nail Clipper 14 Hiker Wood 21 Huntsman Navy Camouflage ACCESSOIRES 48 Couteau de poche – jouet GRANDS COUTEAUX DE POCHE 18 Skipper Pro 21 Skipper Navy Camouflage 24 Wine Master 27 Hunter Pro 31 Hunter Pro M Alox 34 Hunter Pro Alox 3 NAIL CLIP 580 SET LAISSEZ VOS MAINS PARLER POUR VOUS Nous nous exprimons autant par les gestes que par la parole. Les gestes et le langage corporel sont d’importants moyens de communication. C’est pourquoi vos mains doivent être impeccables, tant pour frapper le sac de boxe de votre salle de sport que pour accueillir de nouveaux collègues de bureau. -
Couteaux Certifiés Par La
CC001 Flat size: 13.8125” x 8.5” Fold size: 3.5” x 8.5” ESPAÑOL • Mueva el cuchillo hacia abajo y por todo el afilador en un ligero arco, llevando el mango hacia usted. Repita el procedimiento del otro lado del afilador. EasySteel™ Uso y cuidado de la línea de cuchillos • Reitere estos pasos de 3 a 5 veces, alternando entre el lado derecho78000 e comerciales Chicago Cutlery izquierdo del filo. ® • Capacite a sus empleados en el uso seguro de los cuchillos y en las ™ prácticas laborales seguras para afilarlos. Afilador EasySteel • Use un cuchillo adecuado para cada tarea y para el alimento que esté Cómo usar el afilador EasySteel™ cortando. 1. Traccione el cuchillo desde el final hasta la punta presionando ligeramente • Mantenga los cuchillos afilados. hacia abajo. (No empuje el cuchillo hasta el fondo para después moverlo). • Corte sobre una superficie estable. 2. La cuchilla debe pasar completa… la varilla debe moverse desde la ® Easy Steel™ EasySteel™ 78000 • Lave los cuchillos con cuidado. posición de reposo (el final de la cuchilla)78000 hasta la parte superior de la ® • Al transportar un cuchillo, la cuchilla debe apuntar hacia abajo. posición elevada (punta de la cuchilla.) ® • Después de usarlos, guarde los cuchillos de forma segura, es decir, en una 3. Haga de 1 a 3 pasadas en cada uso. vaina o recipiente. 4. Repita el proceso después de 2-4 cortes. ENGLISH • Use elementos de protección cuando sea necesario. Para deshuesar, es recomendable usar un guante protector firme en la mano que no sujeta el cuchillo, además de un delantal resistente. -
Brushless Multi-Tool Outil Multifonction Sans Balai Herramienta Multiuso Sin Escobillas
Owner’s Manual Guide d’utilisation Manual del propietario Model/ Modelo/ Modèle: OS592701 TM Brushless Multi-Tool Outil multifonction sans balai Herramienta multiuso sin escobillas WARNING: To reduce the risk of injury, the user must read and understand the Owner’s Manual before using this product. Save these instructions for future reference. AVERTISSEMENT : Afin de réduire les risques de blessure, l’utilisateur doit lire et comprendre le guide d’utilisation avant d’utiliser cet article. Conservez le présent guide afin de pouvoir le consulter ultérieurement. ADVERTENCIA : Para reducir el riesgo de lesiones, el usuario debe leer y comprender el Manual del operador antes de utilizar este producto. Guarde estas instrucciones para consultarlas en caso sea necesario. For Customer Service Pour le service à la clientèle OR Servicio al cliente 1-877-SKIL-999 www.skil.com TABLE OF CONTENTS General Power Tool Safety Warnings . 3-5 Safety Warnings for Multi-Tool . 5 Symbols . 6-9 Get to Know Your Multi-Tool . 10 Specifications . 10-11 Operating Instructions . 12-21 Maintenance . 22 Troubleshooting . 22 Limited Warranty of SKIL Cordless Tool . 23 WARNING • Some dust created by power sanding, sawing, grinding, drilling and other construction activities contains chemicals known to the State of California to cause cancer, birth defects or other reproductive harm. Some examples of these chemicals are: – Lead from lead-based paints. – Crystalline silica from bricks, cement, and other masonry products. – Arsenic and chromium from chemically-treated lumber. • Your risk from these exposures varies, depending upon how often you do this type of work. To reduce your exposure to these chemicals: – Work in a well-ventilated area. -
Premier Classic Sora Kanso Classic
Hollow Ground Kiritsuke 6’ Kiritsuke 8” Kiritsuke à lame alvéolé 15,2 cm Kiritsuke 20,3 cm Sora Kanso Classic [ DM0779 ] * [ DM0771 ] 15 Years of Proprietary Composite Blade Technology Solid AUS10A—high-carbon, vanadium stainless 69 layer construction (damascus cladding + proprietary Premier Technologie exclusive de lame composite steel with Heritage fi nish VG-MAX cutting core) Hollow Ground Chef’s 6” Offset Bread 8.25” 69 layer construction (damascus cladding + proprietary Solide AUS10A, haut carbone, l’acier inoxydable Structure de 69 couches (revêtement en acier de Damas Du chef à lame alvéolé 15,2 cm À pain latéral 21 cm VG-MAX cutting core) 3 layer san mai construction * Structure de 69 couches (revêtement en acier de Damas vanadium, avec fi nition de Héritage en plus d’un noyau exclusif VG-MAX) [ DM0747 ] [ DM0724 ] Shun (cladding + VG10 cutting core) en plus d’un noyau exclusif VG-MAX) Structure san mai à 3 couches The Shun-sharp 16° edge (each side) Double-bevel, flat-ground blade Western Chef’s Knife 6” Hollow Ground Slicing 9” Hammered tsuchime fi nish (revêtement, en plus d’un noyau VG10) Tranchant effi lé Shun de 16° (de chaque côté) Lame plate à double biseau Du chef, occidentale 15,2 cm À trancher à lame [ DM0904 ] * Fini tsuchime martelé The Shun-sharp 16° edge (each side) Double-bevel, flat-ground blade The Shun-sharp 16° edge (each side) alvéolé 22,9 cm Tranchant effi lé Shun de 16° (de chaque côté) Lame plate à double biseau Tranchant effi lé Shun de 16 ° (de chaque côté) Serrated Utility 6” [ DM0720 ] The Shun-sharp -
Exoplanet.Eu Catalog Page 1 # Name Mass Star Name
exoplanet.eu_catalog # name mass star_name star_distance star_mass OGLE-2016-BLG-1469L b 13.6 OGLE-2016-BLG-1469L 4500.0 0.048 11 Com b 19.4 11 Com 110.6 2.7 11 Oph b 21 11 Oph 145.0 0.0162 11 UMi b 10.5 11 UMi 119.5 1.8 14 And b 5.33 14 And 76.4 2.2 14 Her b 4.64 14 Her 18.1 0.9 16 Cyg B b 1.68 16 Cyg B 21.4 1.01 18 Del b 10.3 18 Del 73.1 2.3 1RXS 1609 b 14 1RXS1609 145.0 0.73 1SWASP J1407 b 20 1SWASP J1407 133.0 0.9 24 Sex b 1.99 24 Sex 74.8 1.54 24 Sex c 0.86 24 Sex 74.8 1.54 2M 0103-55 (AB) b 13 2M 0103-55 (AB) 47.2 0.4 2M 0122-24 b 20 2M 0122-24 36.0 0.4 2M 0219-39 b 13.9 2M 0219-39 39.4 0.11 2M 0441+23 b 7.5 2M 0441+23 140.0 0.02 2M 0746+20 b 30 2M 0746+20 12.2 0.12 2M 1207-39 24 2M 1207-39 52.4 0.025 2M 1207-39 b 4 2M 1207-39 52.4 0.025 2M 1938+46 b 1.9 2M 1938+46 0.6 2M 2140+16 b 20 2M 2140+16 25.0 0.08 2M 2206-20 b 30 2M 2206-20 26.7 0.13 2M 2236+4751 b 12.5 2M 2236+4751 63.0 0.6 2M J2126-81 b 13.3 TYC 9486-927-1 24.8 0.4 2MASS J11193254 AB 3.7 2MASS J11193254 AB 2MASS J1450-7841 A 40 2MASS J1450-7841 A 75.0 0.04 2MASS J1450-7841 B 40 2MASS J1450-7841 B 75.0 0.04 2MASS J2250+2325 b 30 2MASS J2250+2325 41.5 30 Ari B b 9.88 30 Ari B 39.4 1.22 38 Vir b 4.51 38 Vir 1.18 4 Uma b 7.1 4 Uma 78.5 1.234 42 Dra b 3.88 42 Dra 97.3 0.98 47 Uma b 2.53 47 Uma 14.0 1.03 47 Uma c 0.54 47 Uma 14.0 1.03 47 Uma d 1.64 47 Uma 14.0 1.03 51 Eri b 9.1 51 Eri 29.4 1.75 51 Peg b 0.47 51 Peg 14.7 1.11 55 Cnc b 0.84 55 Cnc 12.3 0.905 55 Cnc c 0.1784 55 Cnc 12.3 0.905 55 Cnc d 3.86 55 Cnc 12.3 0.905 55 Cnc e 0.02547 55 Cnc 12.3 0.905 55 Cnc f 0.1479 55 -
Introduction to Baking and Pastries Chef Tammy Rink with William R
Introduction to Baking and Pastries Chef Tammy Rink With William R. Thibodeaux PH.D. ii | Introduction to Baking and Pastries Introduction to Baking and Pastries | iii Introduction to Baking and Pastries Chef Tammy Rink With William R. Thibodeaux PH.D. iv | Introduction to Baking and Pastries Introduction to Baking and Pastries | v Contents Preface: ix Introduction to Baking and Pastries Topic 1: Baking and Pastry Equipment Topic 2: Dry Ingredients 13 Topic 3: Quick Breads 23 Topic 4: Yeast Doughs 27 Topic 5: Pastry Doughs 33 Topic 6: Custards 37 Topic 7: Cake & Buttercreams 41 Topic 8: Pie Doughs & Ice Cream 49 Topic 9: Mousses, Bavarians and Soufflés 53 Topic 10: Cookies 56 Notes: 57 Glossary: 59 Appendix: 79 Kitchen Weights & Measures 81 Measurement and conversion charts 83 Cake Terms – Icing, decorating, accessories 85 Professional Associations 89 vi | Introduction to Baking and Pastries Introduction to Baking and Pastries | vii Limit of Liability/disclaimer of warranty and Safety: The user is expressly advised to consider and use all safety precautions described in this book or that might be indicated by undertaking the activities described in this book. Common sense must also be used to avoid all potential hazards and, in particular, to take relevant safety precautions concerning likely or known hazards involving food preparation, or in the use of the procedures described in this book. In addition, while many rules and safety precautions have been noted throughout the book, users should always have adult supervision and assistance when working in a kitchen or lab. Any use of or reliance upon this book is at the user's own risk. -
SILICON and OXYGEN ABUNDANCES in PLANET-HOST STARS Erik Brugamyer, Sarah E
The Astrophysical Journal, 738:97 (11pp), 2011 September 1 doi:10.1088/0004-637X/738/1/97 C 2011. The American Astronomical Society. All rights reserved. Printed in the U.S.A. SILICON AND OXYGEN ABUNDANCES IN PLANET-HOST STARS Erik Brugamyer, Sarah E. Dodson-Robinson, William D. Cochran, and Christopher Sneden Department of Astronomy and McDonald Observatory, University of Texas at Austin, 1 University Station C1400, Austin, TX 78712, USA; [email protected] Received 2011 February 4; accepted 2011 June 22; published 2011 August 16 ABSTRACT The positive correlation between planet detection rate and host star iron abundance lends strong support to the core accretion theory of planet formation. However, iron is not the most significant mass contributor to the cores of giant planets. Since giant planet cores are thought to grow from silicate grains with icy mantles, the likelihood of gas giant formation should depend heavily on the oxygen and silicon abundance of the planet formation environment. Here we compare the silicon and oxygen abundances of a set of 76 planet hosts and a control sample of 80 metal-rich stars without any known giant planets. Our new, independent analysis was conducted using high resolution, high signal-to-noise data obtained at McDonald Observatory. Because we do not wish to simply reproduce the known planet–metallicity correlation, we have devised a statistical method for matching the underlying [Fe/H] distributions of our two sets of stars. We find a 99% probability that planet detection rate depends on the silicon abundance of the host star, over and above the observed planet–metallicity correlation. -
Pauline and Other Studies
PAULINE AND OTHER STUDIES IN EARLY CHRISTIAN HISTORY BY W. M. RAM SAY, HoN. D.C.L., ETC. PROF~~SOR OF HUMANITY IN THE UNIVERSITY OF ABERDEEN HODDER AND STOUGHTON LONDON MCMVI VI THE PERMANENCE OF RELIGION AT HOLY PLACES IN WESTERN ASIA II Tomb of a Christian Virgin of the Third Cent).lry (see p. 298). VI THE PERMANENCE OF RELIGION AT HOLY PLACES IN WESTERN ASIA IN the preceding article in this volume, describing the origin of the Ephesian cult of the Mother of God, the permanent attachment of religious awe to special localities was briefly mentioned. In that cult we found a survival or revival of the old paganism of Ephesus, viz., the worship of the Virgin Mother of Artemis. The persistence of those ancient be liefs and rites at the chief centres of paganism exercised so pro found an influence on the history of Christianity in Asia Minor, that it is well to give a more detailed account of the facts, though even this account can only be a brief survey of a few examples selected almost by chance out of the in numerable cases which occur in all parts of the country. I shall take as the foundation of this article a paper read to the Oriental Congress held at London in autumn, 1902, and buried in the Transactions of the Congress, developing and improving the ideas expressed in that paper, and enlarging the number of examples. The strength of the old pagan beliefs did not escape the attention of the Apostle Paul; and his views on the subject affected his action as a missionary in the cities of Asia Minor; and can be traced in his letters. -
IAU Division C Working Group on Star Names 2019 Annual Report
IAU Division C Working Group on Star Names 2019 Annual Report Eric Mamajek (chair, USA) WG Members: Juan Antonio Belmote Avilés (Spain), Sze-leung Cheung (Thailand), Beatriz García (Argentina), Steven Gullberg (USA), Duane Hamacher (Australia), Susanne M. Hoffmann (Germany), Alejandro López (Argentina), Javier Mejuto (Honduras), Thierry Montmerle (France), Jay Pasachoff (USA), Ian Ridpath (UK), Clive Ruggles (UK), B.S. Shylaja (India), Robert van Gent (Netherlands), Hitoshi Yamaoka (Japan) WG Associates: Danielle Adams (USA), Yunli Shi (China), Doris Vickers (Austria) WGSN Website: https://www.iau.org/science/scientific_bodies/working_groups/280/ WGSN Email: [email protected] The Working Group on Star Names (WGSN) consists of an international group of astronomers with expertise in stellar astronomy, astronomical history, and cultural astronomy who research and catalog proper names for stars for use by the international astronomical community, and also to aid the recognition and preservation of intangible astronomical heritage. The Terms of Reference and membership for WG Star Names (WGSN) are provided at the IAU website: https://www.iau.org/science/scientific_bodies/working_groups/280/. WGSN was re-proposed to Division C and was approved in April 2019 as a functional WG whose scope extends beyond the normal 3-year cycle of IAU working groups. The WGSN was specifically called out on p. 22 of IAU Strategic Plan 2020-2030: “The IAU serves as the internationally recognised authority for assigning designations to celestial bodies and their surface features. To do so, the IAU has a number of Working Groups on various topics, most notably on the nomenclature of small bodies in the Solar System and planetary systems under Division F and on Star Names under Division C.” WGSN continues its long term activity of researching cultural astronomy literature for star names, and researching etymologies with the goal of adding this information to the WGSN’s online materials.