Goddard Space Light Center JANUARY4,1 I
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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. -
N O T I C E This Document Has Been Reproduced From
N O T I C E THIS DOCUMENT HAS BEEN REPRODUCED FROM MICROFICHE. ALTHOUGH IT IS RECOGNIZED THAT CERTAIN PORTIONS ARE ILLEGIBLE, IT IS BEING RELEASED IN THE INTEREST OF MAKING AVAILABLE AS MUCH INFORMATION AS POSSIBLE P993-198422 International Collogium on Atomic Spectra and Oscillator Strengths for Astrophysical and Laboratory Plasmas (4th) Held at the National institute of Standards and Technology Gaithersburg, Maryland on September 14-17, 1992 (U.S.) National inst. of Standards and Technology (PL) Gaithersburg, MD Apr 93 US. DEPARTMENT OF COMMERCE Ndioul Techcical IMermeNON Service B•11G 2-10i1A2 2 MIST-1 /4 U.S. VZPARTMENT OF COMMERCE (REV. NATIONAL INSTITUTE OF STANDARDS AND TECHNOLOGY M GONTSOLw1N^BENN O4" COMM 4M /. MANUSCRIPT REVIEW AND APPROVAL "KIST/ p-850 ^' THIS NSTRUCTWNS: ATTACH ORIGINAL OF FORM TO ONE (1) COPY OF MANUSCIIN IT AND SEINE TO: PUBLICATIOM OATS NUMBER PRINTED PAGES April 1993 199 HE SECRETAIIY, APPROPRIATE EDITO RIAL REVIEW BOARD. ITLE AND SUBTITLE (CITE NN PULL) 4rh International Colloquium on Atomic Spectra and Oscillator Strengths for Astrophysical and Laboratory Plasmas -- POSTER PAPERS :ONTIEACT OR GRANT NUMBER TYPE OF REPORT AND/OR PERIOD COMM UTHOR(S) (LAST %,TAME, POST NNITIAL, SECOND INITIAL) PERFORM" ORGANIZATION (CHECK (IQ ONE SOX) EDITORS XXX MIST/GAITHERSBUIIG Sugar, Jack and Leckrone, B:;vid INST/BODUM JILA BOIRDE11 "ORATORY AND DIVISION NAMES (FIRST MOST AUTHOR ONLY) Physics Laboratory/Atomic Physics Division 'PONSORING ORGANIZATION NAME AND COMPLETE ADDRESS TREET, CITY. STATE. ZNh ^y((S/ ,T AiL7A - -ASO IECOMMENDsO FOR MIST PUBLICATION JOVIAMAL OF RESEMICM (MIST JRES) CIONOGRAPK (MIST MN) LETTER CIRCULAR J. PHYS. A CHEM. -
Frontier: First Encounters 2 Contents
Frontier: First Encounters 2 Contents Credits v Preface vii Quick start ix 1 Tutorial 1 1.1 Your first view . 1 1.2 You and your ship (Inventory mode) . 2 1.3 The galaxy . 3 1.4 Where to go, and what to do there . 5 1.5 Getting out of here . 9 1.6 Arriving . 11 1.7 On landing . 14 2 The controls 17 2.1 Welcome to your Saker Mk III . 17 2.2 Ship instrumentation, and how to use it . 17 2.3 The View Panel (F1) . 19 2.4 The Inventory Panel (F2) . 22 2.5 The Map Panel (F3) . 25 2.6 The Communications Panel (F4) . 28 2.7 The Scanner . 30 2.8 Fuel Gauge and Temperature Gauges . 31 2.9 Warning Lights . 31 2.10 Dual Console . 32 2.11 Options . 35 3 Flying a spacecraft 37 3.1 Basic flight controls . 37 3.2 Fly-by-wire — an idiot’s guide . 38 3.3 Launching and docking procedures . 39 3.4 Flying between star-systems . 44 3.5 Flying within a system . 46 3.6 Intra-system flight without an autopilot . 49 3.7 Manual flight, and relative velocities . 51 3.8 Your pilot’s test — a revision guide . 55 3.9 Basic combat controls . 57 i ii CONTENTS 3.10 The combat drill . 59 3.11 Combat techniques . 63 3.12 Interception techniques . 68 3.13 Planetary combat . 70 3.14 Full manual flight control (Advanced) . 73 4 Careers 77 4.1 Bulletin Boards . 77 4.2 Deliveries . 79 4.2.1 Parcel courier . -
The X-Ray Universe 2017
The X-ray Universe 2017 6−9 June 2017 Centro Congressi Frentani Rome, Italy A conference organised by the European Space Agency XMM-Newton Science Operations Centre National Institute for Astrophysics, Italian Space Agency University Roma Tre, La Sapienza University ABSTRACT BOOK Oral Communications and Posters Edited by Simone Migliari, Jan-Uwe Ness Organising Committees Scientific Organising Committee M. Arnaud Commissariat ´al’´energie atomique Saclay, Gif sur Yvette, France D. Barret (chair) Institut de Recherche en Astrophysique et Plan´etologie, France G. Branduardi-Raymont Mullard Space Science Laboratory, Dorking, Surrey, United Kingdom L. Brenneman Smithsonian Astrophysical Observatory, Cambridge, USA M. Brusa Universit`adi Bologna, Italy M. Cappi Istituto Nazionale di Astrofisica, Bologna, Italy E. Churazov Max-Planck-Institut f¨urAstrophysik, Garching, Germany A. Decourchelle Commissariat ´al’´energie atomique Saclay, Gif sur Yvette, France N. Degenaar University of Amsterdam, the Netherlands A. Fabian University of Cambridge, United Kingdom F. Fiore Osservatorio Astronomico di Roma, Monteporzio Catone, Italy F. Harrison California Institute of Technology, Pasadena, USA M. Hernanz Institute of Space Sciences (CSIC-IEEC), Barcelona, Spain A. Hornschemeier Goddard Space Flight Center, Greenbelt, USA V. Karas Academy of Sciences, Prague, Czech Republic C. Kouveliotou George Washington University, Washington DC, USA G. Matt Universit`adegli Studi Roma Tre, Roma, Italy Y. Naz´e Universit´ede Li`ege, Belgium T. Ohashi Tokyo Metropolitan University, Japan I. Papadakis University of Crete, Heraklion, Greece J. Hjorth University of Copenhagen, Denmark K. Poppenhaeger Queen’s University Belfast, United Kingdom N. Rea Instituto de Ciencias del Espacio (CSIC-IEEC), Spain T. Reiprich Bonn University, Germany M. Salvato Max-Planck-Institut f¨urextraterrestrische Physik, Garching, Germany N. -
Today Our Place in the Universe
Our place in the Universe , and other sources ully T , Bob Patterson, Donna Cox (NCSA), Data: Hipparcos, Brent iz: Stuart Levy V Tom Abel Today KIPAC The Birth, Life & Aftermath of the First Stars Tom Abel KIPAC/Stanford work with Matt Turk (Birth) John Wise (Life) Ralf Kähler (Scientific Visualization) Outline • Conception • A difficult birth • A surprising life • Remarkable consequences • Three-D radiation transport around point sources • Spatially & temporally structured adaptive cosmological & relativistic hydrodynamics • public version of enzo at: http://lca.ucsd.edu/portal/software/enzo Discovery by How we find things: Computer? 6 6.28 Conception Physics problem: • Initial Conditions: COBE/ACBAR/ Boomerang/WMAP/CfA/SDDS/ 2DF/CDMS/DAMA/Edelweiss/... + Theory: Constituents, Density Fluctuations, Thermal History • Physics: Gravity, MHD, Chemistry, Radiative Cooling, Radiation Transport, Cosmic Rays, Dust drift & cooling, Supernovae, Stellar evolution, etc. Ralf Kähler & Tom Abel for PBS • Transition from Linear to Non- Origins. Aired Dec 04 Linear: • Using patched based structured adaptive (space & time) mesh refinement Making a proto-star Simulation: Tom Abel (KIPAC/Stanford), Greg Bryan (Columbia), Mike Norman (UCSD) Viz: Ralf Kähler (AEI, ZIB, KIPAC), Bob Patterson, Stuart Levy, Donna Cox (NCSA), Tom Abel © “The Unfolding Universe” Discovery Channel 2002 Dynamic range ~1e12. Typically 3 solar mass dm particles > 30 levels of refinement > 8 cells per local Jeans Length tens of thousands of grid patches non-equilibrium chemistry dynamically load balanced RT effects above 1e12 cm-3 Zoom in MPI. 16 processors enough Turk & Abel in prep Note disks within disks happen routinely in turbulent collapses! Mass Scales? Kelvin Helmholtz time at ZAMS Abel, Bryan & Norman 2002 Recap First Stars are isolated and very massive • Theoretical uncertainty: 30 - 300 solar mass Many simulations with three different numerical techniques and a large range of numerical resolutions have converged to this result. -
Publications Ofthe Astronomical Society Ofthe Pacific 99:490-496, June 1987
Publications ofthe Astronomical Society ofthe Pacific 99:490-496, June 1987 RADIAL VELOCITIES OF M DWARF STARS GEOFFREY W. MARCY,* VICTORIA LINDSAY,* AND KAREN WILSON Department of Physics and Astronomy, San Francisco State University, San Francisco, California 94132 Received 1987 February 26, revised 1987 March 28 ABSTRACT Radial velocities for 72 M dwarfs have been obtained having internal errors of about 0.1 km s1 and external errors of about 0.4 km s_1. Multiple velocity measurements of ten dMe stars have yielded a set of six which have no stellar companions, providing confirmation that the dMe phenomenon can occur in single stars. These single dMe stars have low space motions indicative of relative youth. Four stars from the entire survey were found to have double-line spectra and two were found to be single-line spectroscopic binaries of low amplitude. The zero point of the velocity scale is found to agree well with that of O. C. Wilson (1967) and differences are noted among other radial-velocity studies. Most of the stars in this study have velocities sufficiently well determined to constitute potential radial-velocity standards. Key words: K-M dwarfs-radial velocities I. Introduction atic difference between their velocities and O. C. 1 Accurate measurements of radial velocities for M Wilson's of —1.7 km s , a discrepancy not explainable by dwarfs are used to address a number of astrophysical the random errors of the two studies. problems such as the age dependence of the kinematics of Thus, it is not known at present which zero point is to the Galaxy (cf. -
October, 2011
IN THIS ISSUE: OCTOBER 2011 Event Calendar, News Notes Minutes of the September Meeting MVAS Reminders: Party-on MVAS Activities: On The Road Again Observer’s Notes: Variable Heroines MVAS Homework: M-76, Little Dumbbell Homework Charts: Algol, asteroid (15) Eunomia Constellation of the Month: Perseus November 2011 Sky Almanac Gallery: Comet Quest, Summer Photos Meteorite Editor: Phil Plante 1982 Mathews Rd. #2 Youngstown OH 44514 OCTOBER 2011 NEWS NOTES Newsletter of the Mahoning Valley Astronomical Society, Inc. The Big Ear. Lofar (Low Frequency Array) is a new kind of radio telescope. It can see radio waves with low frequencies, similar to those that give us FM radio. Rather than collecting MVAS CALENDAR signals from individual radio sources, Lofar continuously monitors large swathes of sky. Lofar is more sensitive to the OCT 22 Business meeting at the MVCO 8:00 PM longest observable radio waves than any other telescope. It can OCT 29 Halloween Party at the MVCO 7:00 PM see many billions of light years out into space, back to the time before the first stars formed, a few hundred million years after NOV17/18 Leonid Meteor watch. On your own? Midnight… the Big Bang. On Monday, September 21, 2011, Sweden's Minister for Education and Research, Jan Bjorklund, opened the NOV 19 Business meeting at YSU. Show at 8:00 PM Onsala Space Observatory's newest telescope; to become part NOV 26 Star Party at the MVCO. 7:00 PM till…. of Lofar, which is the world's largest radio telescope. The 192 new radio antennas at Onsala's Lofar station will be linked together with 47 similar stations over the whole of NATIONAL & REGIONAL EVENTS Europe, and sent over the Internet to a central supercomputer in OCT 24 - 30 CSPG Fall Star Party, held in Chiefland, FL . -
September 2020 BRAS Newsletter
A Neowise Comet 2020, photo by Ralf Rohner of Skypointer Photography Monthly Meeting September 14th at 7:00 PM, via Jitsi (Monthly meetings are on 2nd Mondays at Highland Road Park Observatory, temporarily during quarantine at meet.jit.si/BRASMeets). GUEST SPEAKER: NASA Michoud Assembly Facility Director, Robert Champion What's In This Issue? President’s Message Secretary's Summary Business Meeting Minutes Outreach Report Asteroid and Comet News Light Pollution Committee Report Globe at Night Member’s Corner –My Quest For A Dark Place, by Chris Carlton Astro-Photos by BRAS Members Messages from the HRPO REMOTE DISCUSSION Solar Viewing Plus Night Mercurian Elongation Spooky Sensation Great Martian Opposition Observing Notes: Aquila – The Eagle Like this newsletter? See PAST ISSUES online back to 2009 Visit us on Facebook – Baton Rouge Astronomical Society Baton Rouge Astronomical Society Newsletter, Night Visions Page 2 of 27 September 2020 President’s Message Welcome to September. You may have noticed that this newsletter is showing up a little bit later than usual, and it’s for good reason: release of the newsletter will now happen after the monthly business meeting so that we can have a chance to keep everybody up to date on the latest information. Sometimes, this will mean the newsletter shows up a couple of days late. But, the upshot is that you’ll now be able to see what we discussed at the recent business meeting and have time to digest it before our general meeting in case you want to give some feedback. Now that we’re on the new format, business meetings (and the oft neglected Light Pollution Committee Meeting), are going to start being open to all members of the club again by simply joining up in the respective chat rooms the Wednesday before the first Monday of the month—which I encourage people to do, especially if you have some ideas you want to see the club put into action. -
GRAVITY ASTROPHYSICS a Plan for the 1990S
ULTRAVIOLET, VISIBLE, and GRAVITY ASTROPHYSICS A Plan for the 1990s (NASA-NP-I52) ULTRAVIOLET, N94-24973 VISI3LE, ANO GRAVITY ASTROPHYSICS: A PLAN FOR THE 1990'S (NASA) 76 p Unclas HI190 0207794 ORIGINAL PAGE COLOR PHOTOGRAPH National Aeronautics and Space Administration I-oreword N ASA'sprioritiesOfficefrom oftheSpaceU.S. NationalScience Academyand Applicationsof Sciences.(OSSA)Guidancereceivesto theadviceOSSAon Astrophysicsscientific strategyDivision,and in particular, is provided by dedicated Academy committees, ad hoc study groups and, at 10-year intervals, by broadly mandated astronomy and astrophysics survey committees charged with making recommen- dations for the coming decade. Many of the Academy's recommendations have important implications for the conduct of ultraviolet and visible-light astronomy from space. Moreover, these areas are now poised for an era of rapid growth. Through technological progress, ultraviolet astronomy has already risen from a novel observational technique four decades ago to the mainstream of astronomical research today. Recent developments in space technology and instrumen- tation have the potential to generate comparably dramatic strides in observational astronomy within the next 10 years. In 1989, the Ultraviolet and Visible Astrophysics Branch of the OSSA Astrophysics Division recognized the need for a new, long-range plan that would implement the Academy's recommendations in a way that yielded the most advantageous use of new technology. NASA's Ultraviolet, Visible, and Gravity Astrophysics Management Operations Working Group was asked to develop such a plan for the 1990s. Since the Branch holds programmatic responsibility for space research in gravitational physics and relativity, as well as for ultraviolet and visible-light astrophysics, missions in those areas were also included. -
More Than a Vulture: a Response to Sweatman and Tsikritsis
Mediterranean Archaeology and Archaeometry, Vol. 17, No 2, (2017), pp. 57-74 Copyright © 2017 MAA Open Access. Printed in Greece. All rights reserved. DOI: 10.5281/zenodo.581724 MATTERS ARISING DECODING GÖBEKLI TEPE WITH ARCHAEOASTRONOMY: WHAT DOES THE FOX SAY?” by Sweatman, M.B. and D. Tsikritsis MORE THAN A VULTURE: A RESPONSE TO SWEATMAN AND TSIKRITSIS By Jens Notroff, Oliver Dietrich, Laura Dietrich, Cecilie Lelek Tvetmarken, Moritz Kinzel, Jonas Schlindwein, Devrim Sönmez, Lee Clare CRITICAL EVALUATION OF THE PAPER BY SWEATMAN, M. B. AND D. TSIKRITSIS, “DECODING GÖBEKLI TEPE WITH ARCHAEOASTRONOMY: WHAT DOES THE FOX SAY?” by Paul D. Burley MORE THAN A VULTURE: A RESPONSE TO SWEATMAN AND TSIKRITSIS Jens Notroff1, Oliver Dietrich1, Laura Dietrich1, Cecilie Lelek Tvetmarken1, Moritz Kinzel2, Jonas Schlindwein1, Devrim Sönmez3, Lee Clare1 1Deutsches Archäologisches Institut, Orient-Abteilung, Podbielskiallee 69–71, D-14195 Berlin, Germany 2Carsten Niebuhr Centre for Multicultural Heritage Department of Cross-Cultural and Regional Studies – ToRS University of Copenhagen, Karen Blixen Plads 8, DK-2300 Copenhagen S, Denmark 3Deutsches Archäologisches Institut, Abteilung Istanbul, Inönü Caddesi 10 TR-34437 Gümüssuyu-Istanbul, Turkey Received: 28/04/2017 Accepted: 01/05/2017 Corresponding author: Jens Notroff ([email protected]) ABSTRACT In a paper recently published in this journal, Martin B. Sweatman and Dimitrios Tsikritsis from the Universi- ty of Edinburgh (School of Engineering) have suggested an interpretation for the early Neolithic monumen- tal enclosures at Göbekli Tepe as space observatories and the site's complex iconography the commemora- tion of a catastrophic astronomical event ('Younger Dryas Comet Impact'). As the archaeologists excavating this site, we would like to comment on a few points that we feel require consideration in this discussion. -
Solar Writer Report for Abraham Lincoln
FIXED STARS A Solar Writer Report for Abraham Lincoln Written by Diana K Rosenberg Compliments of:- Stephanie Johnson Seeing With Stars Astrology PO Box 159 Stepney SA 5069 Australia Tel/Fax: +61 (08) 8331 3057 Email: [email protected] Web: www.esotech.com.au Page 2 Abraham Lincoln Natal Chart 12 Feb 1809 12:40:56 PM UT +0:00 near Hodgenville 37°N35' 085°W45' Tropical Placidus 22' 13° 08°ˆ ‡ 17' ¾ 06' À ¿É ‰ 03° ¼ 09° 00° 06° 09°06° ˆ ˆ ‡ † ‡ 25° 16' 41'08' 40' † 01' 09' Œ 29' ‰ 9 10 23° ¶ 8 27°‰ 11 Ï 27° 01' ‘ ‰02' á 7 12 ‘ áá 23° á 23° ¸ 23°Š27' á Š à „ 28' 28' 6 18' 1 10°‹ º ‹37' 13° 05' ‹ 5 Á 22° ½ 27' 2 4 01' Ü 3 07° Œ ƒ » 09' 23° 09° Ý Ü 06° 16' 06' Ê 00°ƒ 13° 22' Ý 17' 08°‚ Page 23 Astrological Summary Chart Point Positions: Abraham Lincoln Planet Sign Position House Comment The Moon Capricorn 27°Cp01' 12th The Sun Aquarius 23°Aq27' 12th read into 1st House Mercury Pisces 10°Pi18' 1st Venus Aries 7°Ar27' 1st read into 2nd House Mars Libra 25°Li29' 8th Jupiter Pisces 22°Pi05' 1st Saturn Sagittarius 3°Sg08' 9th read into 10th House Uranus Scorpio 9°Sc40' 8th Neptune Sagittarius 6°Sg41' 9th read into 10th House Pluto Pisces 13°Pi37' 1st The North Node Scorpio 6°Sc09' 8th The South Node Taurus 6°Ta09' 2nd The Ascendant Aquarius 23°Aq28' 1st The Midheaven Sagittarius 8°Sg22' 10th The Part of Fortune Capricorn 27°Cp02' 12th Chart Point Aspects Planet Aspect Planet Orb App/Sep The Moon Square Mars 1°32' Separating The Moon Conjunction The Part of Fortune 0°00' Applying The Sun Trine Mars 2°02' Applying The Sun Conjunction The Ascendant -
Patrick Moore's Practical Astronomy Series
Patrick Moore’s Practical Astronomy Series Other Titles in this Series Telescopes and Techniques (2nd Edn.) Observing the Planets Chris Kitchin Peter T. Wlasuk The Art and Science of CCD Astronomy Light Pollution David Ratledge (Ed.) Bob Mizon The Observer’s Year Using the Meade ETX Patrick Moore Mike Weasner Seeing Stars Practical Amateur Spectroscopy Chris Kitchin and Robert W. Forrest Stephen F. Tonkin (Ed.) Photo-guide to the Constellations More Small Astronomical Observatories Chris Kitchin Patrick Moore (Ed.) The Sun in Eclipse Observer’s Guide to Stellar Evolution Michael Maunder and Patrick Moore Mike Inglis Software and Data for Practical Astronomers How to Observe the Sun Safely David Ratledge Lee Macdonald Amateur Telescope Making The Practical Astronomer’s Deep-Sky Stephen F. Tonkin (Ed.) Companion Observing Meteors, Comets, Supernovae and Jess K. Gilmour other Transient Phenomena Observing Comets Neil Bone Nick James and Gerald North Astronomical Equipment for Amateurs Observing Variable Stars Martin Mobberley Gerry A. Good Transit: When Planets Cross the Sun Visual Astronomy in the Suburbs Michael Maunder and Patrick Moore Antony Cooke Practical Astrophotography Astronomy of the Milky Way: The Observer’s Jeffrey R. Charles Guide to the Northern and Southern Milky Way Observing the Moon (2 volumes) Peter T. Wlasuk Mike Inglis Deep-Sky Observing The NexStar User Guide Steven R. Coe Michael W. Swanson AstroFAQs Observing Binary and Double Stars Stephen F. Tonkin Bob Argyle (Ed.) The Deep-Sky Observer’s Year Navigating the Night Sky Grant Privett and Paul Parsons Guilherme de Almeida Field Guide to the Deep Sky Objects The New Amateur Astronomer Mike Inglis Martin Mobberley Choosing and Using a Schmidt-Cassegrain Care of Astronomical Telescopes and Telescope Accessories Rod Mollise M.