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Regional Structural Setting of Yucca Mountain, Southwestern Nevada
) i WM RECORD COPY I: // lt- USGS-OFR-84-854 - USGS-OFR-84-854 UNITED STATES DEPARTMENT OF THE INTERIOR GEOLOGICAL SURVEY REGIONAL STRUCTURAL SETTING OF YUCCA MOUNTAIN, SOUTHWESTERN NEVADA, AND LATE CENOZOIC RATES OF TECTONIC ACTIVITY IN PART OF THE SOUTHWESTERN GREAT BASIN, NEVADA AND CALIFORNIA by U. J. Carr 06 : . , CD CD. Open-File Report 84-854 Prepared in cooperation with the Nevada Operations Office U.S. Department of Energy (Interagency Agreement DE-AI08-78ET44802) This report is preliminary and has not been reviewed for-conformity with U.S. Geological Survey editorial standards and stratigraphic nomenclature. Company names are for descriptive purposes only and do not constitute endorsement by the U.S. Geological Survey. Denver, Colorado 1984 ~~- ~ - ~~ ___~~~ Copies of this Open-File Report may be purchased from Open-File Services Secton Branch of Distribution U.S. Geological Survey Box 25425, Federal Center Denver, Colorado 80225 PREPAYMENT IS REQUIRED Price information will be published in the monthly listing 'New Publications of the Geological Survey" FOR ADDITIONAL ORDERING INFORMATION CALL: Commercial: (303) 236-7476 FTS: 776-7476 USGS-OFR-84-854 USGS-OFR-84-854 UNITED STATES DEPARTMENT OF THE INTERIOR GEOLOGICAL SURVEY Denver, Colorado REGIONAL STRUCTURAL SETTING OF YUCCA MOUNTAIN, SOUTHWESTERN NEVADA, AND LATE CENOZOIC RATES OF TECTONIC ACTIVITY IN PART OF THE SOUTHWESTERN GREAT BASIN, NEVADA AND CALIFORNIA by W. J. Carr CONTENTS Page Abstract................................................................... 1 Introduction.................................................................................................. 4 Structural-physiographic subsections of the southwestern Great Basin ....... 9 Walker Lane belt ........................................ ...... ** 9 Basin-range subsection ..................................................21 Inyo-Mono subsection ............................................................26 Boundary between Inyo-Mono and Walker Lane belt subsections ...... -
2017 Býk Otec Fir 2016 Býk Otec Fir 2015 Býk
2017 BÝK OTEC FIR 2016 BÝK OTEC FIR 2015 BÝK OTEC FIR 2014 BÝK OTEC FIR 1 2949 LEGACY FRAZZLED 507 2 2944 NASHVILLE DYNASTY 551 BÝCI REGISTROVANÍ V ČR 3 2933 RIVETING FRAZZLED 614 Aktualizace k: 5.1.2019 1 2920 CHARL CHARLEY 551 BÝCI *2017 a starší. TPI 2400 a více 4 2919 PINNACLE 7 MTS 5 2913 AltaLAWSON AltaROBSON 11 Natural, Zooservis 6 2908 DISCJOCKEY FORTUNE 200 Ostatní 7 2908 FULLMARKS FORTUNE 200 8 2908 EISAKU SAMURI 507 9 2907 ACURA ACHIEVER 29 10 2904 BUNDLE ACHIEVER 29 11 2903 DEDICATE SUPERHERO 551 12 2902 PURSUIT IMAX 200 13 2893 EMERALD FORTUNE 200 14 2893 AltaRNR AltaROBSON 11 15 2889 ROME FRAZZLED 614 16 2883 RENEGADE JALTAOAK 550 17 2883 SOLUTION FRAZZLED 614 18 2883 BATMAN IMAX 200 19 2882 ROYAL DUKE 29 20 2882 PONCHO NOBLE 551 21 2879 CHALLENGER SUPERHERO 200 22 2878 PERK SPECTRE 29 23 2878 CRIMSON SPECTRE 29 24 2876 MAESTRO IMAX 200 25 2874 GAMECHANGER MODESTY 1 26 2873 PYRAMID GUARANTEE 200 27 2873 MENACE DELTA-WORTH 551 28 2872 APPLEBEES ACHIEVER 29 29 2872 CASCADE KING ROYAL 507 30 2870 AltaROBERT AltaROBSON 11 31 2869 ARISTOCRAT FRAZZLED 515 32 2869 RAPID RUBI-HAZE 551 33 2867 AltaROADY AltaROBSON 11 34 2866 BIG AL FRAZZLED 507 35 2866 PETRO PROPHECY 29 36 2866 VALUE DUKE 29 37 2865 NACASH SUPERHERO 180 38 2865 EMBELLISH FORTUNE 200 39 2864 BRASS FRAZZLED 507 40 2861 MESCALERO PINNACLE 250 41 2860 KORBEL ACHIEVER 1 42 2860 TIMBERLAKE IMAX 200 43 2860 AltaHOTJOB HOTLINE 11 44 2859 ENFORCE FRAZZLED 100 45 2858 HEMINGWAY FORTUNE 200 46 2857 EXODUS REASON 250 47 2857 ALERT FORTUNE 200 48 2856 DIVERSITY MEDLEY 29 49 2856 -
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............................................................................................................ -
Petrogenes1.S of Apollo 11 Basalts and Implications
PETROGENES1.S OF APOLLO 11 BASALTS AND IMPLICATIONS FOR LUNAR ORIGIN A, E. Rinqwood Department of Geophysics and Geochemistry Australian National University Canberra ABSTRACT The origin of Apollo 11 basalts is discussed in terms of two hypotheses: (i) formation by a small degree of partial melting in the lunar interior and (ii) formation by prolonged near-surface crystallization differentiation in a lava lake. The second hypoth- esis is rejected on the following grounds: Most Apollo 11 magmas are far removed from the plagioclase-pyroxene-ilmenite cotectic; fractional crystallization cannot explain the large variations in concentrations of incompatible trace elehents in conjunction with the small variations in major element compositions, particularly, _IMg ratios; experimentally determined partition coefficients show Fe Pack3 that the high abundances of Cr and V in Apollo 11 cannot be reconciled A with the previous separation of large quantities of ore minerals and pyroxenes. On the other hand, the major element and trace element jq contents of Apollo 11 rocks can be explained by partial melting of sovvromaterial which buffers the major element compositions and causes enrichments of incompatible elements according to the degree of partial melting( fiisk hypbthesis) Two alternative sources have been suggested for Apollo 11 basalts formed by partial melting: (i) unfractionated pyroxenite source region at depths of 200-600 km, (ii) fractionated source region with incompatible elements (e-g. Ba, U, rare 'earths) strongly enriched over chondritic abundances and containing plagioclase (approximate eucritic composition). Mass balance calculations'and plagioclase stability conditions show that the second hypothesis requires Apollo 1l.basalts to be generated by partial melting in the outer 150 km of the moon. -
Alpha ELT Listing
Lienholder Name Lienholder Address City State Zip ELT ID 1ST ADVANTAGE FCU PO BX 2116 NEWPORT NEWS VA 23609 CFW 1ST COMMAND BK PO BX 901041 FORT WORTH TX 76101 FXQ 1ST FNCL BK USA 47 SHERMAN HILL RD WOODBURY CT 06798 GVY 1ST LIBERTY FCU PO BX 5002 GREAT FALLS MT 59403 ESY 1ST NORTHERN CA CU 1111 PINE ST MARTINEZ CA 94553 EUZ 1ST NORTHERN CR U 230 W MONROE ST STE 2850 CHICAGO IL 60606 GVK 1ST RESOURCE CU 47 W OXMOOR RD BIRMINGHAM AL 35209 DYW 1ST SECURITY BK WA PO BX 97000 LYNNWOOD WA 98046 FTK 1ST UNITED SVCS CU 5901 GIBRALTAR DR PLEASANTON CA 94588 W95 1ST VALLEY CU 401 W SECOND ST SN BERNRDNO CA 92401 K31 360 EQUIP FIN LLC 300 BEARDSLEY LN STE D201 AUSTIN TX 78746 DJH 360 FCU PO BX 273 WINDSOR LOCKS CT 06096 DBG 4FRONT CU PO BX 795 TRAVERSE CITY MI 49685 FBU 777 EQUIPMENT FIN LLC 600 BRICKELL AVE FL 19 MIAMI FL 33131 FYD A C AUTOPAY PO BX 40409 DENVER CO 80204 CWX A L FNCL CORP PO BX 11907 SANTA ANA CA 92711 J68 A L FNCL CORP PO BX 51466 ONTARIO CA 91761 J90 A L FNCL CORP PO BX 255128 SACRAMENTO CA 95865 J93 A L FNCL CORP PO BX 28248 FRESNO CA 93729 J95 A PLUS FCU PO BX 14867 AUSTIN TX 78761 AYV A PLUS LOANS 500 3RD ST W SACRAMENTO CA 95605 GCC A/M FNCL PO BX 1474 CLOVIS CA 93613 A94 AAA FCU PO BX 3788 SOUTH BEND IN 46619 CSM AAC CU 177 WILSON AVE NW GRAND RAPIDS MI 49534 GET AAFCU PO BX 619001 MD2100 DFW AIRPORT TX 75261 A90 ABLE INC 503 COLORADO ST AUSTIN TX 78701 CVD ABNB FCU 830 GREENBRIER CIR CHESAPEAKE VA 23320 CXE ABOUND FCU PO BX 900 RADCLIFF KY 40159 GKB ACADEMY BANK NA PO BX 26458 KANSAS CITY MO 64196 ATF ACCENTRA CU 400 4TH -
Astronomy 2008 Index
Astronomy Magazine Article Title Index 10 rising stars of astronomy, 8:60–8:63 1.5 million galaxies revealed, 3:41–3:43 185 million years before the dinosaurs’ demise, did an asteroid nearly end life on Earth?, 4:34–4:39 A Aligned aurorae, 8:27 All about the Veil Nebula, 6:56–6:61 Amateur astronomy’s greatest generation, 8:68–8:71 Amateurs see fireballs from U.S. satellite kill, 7:24 Another Earth, 6:13 Another super-Earth discovered, 9:21 Antares gang, The, 7:18 Antimatter traced, 5:23 Are big-planet systems uncommon?, 10:23 Are super-sized Earths the new frontier?, 11:26–11:31 Are these space rocks from Mercury?, 11:32–11:37 Are we done yet?, 4:14 Are we looking for life in the right places?, 7:28–7:33 Ask the aliens, 3:12 Asteroid sleuths find the dino killer, 1:20 Astro-humiliation, 10:14 Astroimaging over ancient Greece, 12:64–12:69 Astronaut rescue rocket revs up, 11:22 Astronomers spy a giant particle accelerator in the sky, 5:21 Astronomers unearth a star’s death secrets, 10:18 Astronomers witness alien star flip-out, 6:27 Astronomy magazine’s first 35 years, 8:supplement Astronomy’s guide to Go-to telescopes, 10:supplement Auroral storm trigger confirmed, 11:18 B Backstage at Astronomy, 8:76–8:82 Basking in the Sun, 5:16 Biggest planet’s 5 deepest mysteries, The, 1:38–1:43 Binary pulsar test affirms relativity, 10:21 Binocular Telescope snaps first image, 6:21 Black hole sets a record, 2:20 Black holes wind up galaxy arms, 9:19 Brightest starburst galaxy discovered, 12:23 C Calling all space probes, 10:64–10:65 Calling on Cassiopeia, 11:76 Canada to launch new asteroid hunter, 11:19 Canada’s handy robot, 1:24 Cannibal next door, The, 3:38 Capture images of our local star, 4:66–4:67 Cassini confirms Titan lakes, 12:27 Cassini scopes Saturn’s two-toned moon, 1:25 Cassini “tastes” Enceladus’ plumes, 7:26 Cepheus’ fall delights, 10:85 Choose the dome that’s right for you, 5:70–5:71 Clearing the air about seeing vs. -
Revisiting the Low-Luminosity Galaxy Population of the NGC 5846 Group with SDSS
A&A 511, A12 (2010) Astronomy DOI: 10.1051/0004-6361/200811013 & c ESO 2010 Astrophysics Revisiting the low-luminosity galaxy population of the NGC 5846 group with SDSS P. Eigenthaler and W. W. Zeilinger Institut für Astronomie, Universität Wien, Türkenschanzstraße 17, 1180 Vienna, Austria e-mail: [email protected] Received 22 September 2008 / Accepted 26 November 2009 ABSTRACT Context. Low-luminosity galaxies are known to outnumber the bright galaxy population in poor groups and clusters of galaxies. Yet, the investigation of low-luminosity galaxy populations outside the Local Group remains rare and the dependence on different group environments is still poorly understood. Previous investigations have uncovered the photometric scaling relations of early-type dwarfs and a strong dependence of morphology with environment. Aims. The present study aims to analyse the photometric and spectroscopic properties of the low-luminosity galaxy population in the nearby, well-evolved and early-type dominated NGC 5846 group of galaxies. It is the third most massive aggregate of early-type galaxies after the Virgo and Fornax clusters in the local universe. Photometric scaling relations and the distribution of morphological types as well as the characteristics of emission-line galaxies are investigated. Methods. Spectroscopically selected low-luminosity group members from the Sloan Digital Sky Survey with cz < 3000 km s−1 within aradiusof2◦ = 0.91 Mpc around NGC 5846 are analysed. Surface brightness profiles of early-type galaxies are fit by a Sérsic model ∝r1/n. Star formation rates, oxygen abundances, and emission characteristics are determined for emission-line galaxies. Results. Seven new group members showing no entry in previous catalogues are identified in the outer (>1.33◦) parts of the system. -
A Search For" Dwarf" Seyfert Nuclei. VII. a Catalog of Central Stellar
TO APPEAR IN The Astrophysical Journal Supplement Series. Preprint typeset using LATEX style emulateapj v. 26/01/00 A SEARCH FOR “DWARF” SEYFERT NUCLEI. VII. A CATALOG OF CENTRAL STELLAR VELOCITY DISPERSIONS OF NEARBY GALAXIES LUIS C. HO The Observatories of the Carnegie Institution of Washington, 813 Santa Barbara St., Pasadena, CA 91101 JENNY E. GREENE1 Department of Astrophysical Sciences, Princeton University, Princeton, NJ ALEXEI V. FILIPPENKO Department of Astronomy, University of California, Berkeley, CA 94720-3411 AND WALLACE L. W. SARGENT Palomar Observatory, California Institute of Technology, MS 105-24, Pasadena, CA 91125 To appear in The Astrophysical Journal Supplement Series. ABSTRACT We present new central stellar velocity dispersion measurements for 428 galaxies in the Palomar spectroscopic survey of bright, northern galaxies. Of these, 142 have no previously published measurements, most being rela- −1 tively late-type systems with low velocity dispersions (∼<100kms ). We provide updates to a number of literature dispersions with large uncertainties. Our measurements are based on a direct pixel-fitting technique that can ac- commodate composite stellar populations by calculating an optimal linear combination of input stellar templates. The original Palomar survey data were taken under conditions that are not ideally suited for deriving stellar veloc- ity dispersions for galaxies with a wide range of Hubble types. We describe an effective strategy to circumvent this complication and demonstrate that we can still obtain reliable velocity dispersions for this sample of well-studied nearby galaxies. Subject headings: galaxies: active — galaxies: kinematics and dynamics — galaxies: nuclei — galaxies: Seyfert — galaxies: starburst — surveys 1. INTRODUCTION tors, apertures, observing strategies, and analysis techniques. -
Dr. Sara Seager Exoplanets and the Search for Habitable Worlds June
: Fort Worth Astronomical Society (Est. 1949) May - June 2011 Astronomical League Member May Meeting: Dr. Sara Seager Exoplanets and the Search for Habitable Worlds June Meeting: Harry Bearman Optics In the normal location Club Calendars – 2 Skyportunities – 4 Black Holes – 5 Mercury: The Elusive Planet – 6 Club Reports – 7 Hercules – 8 What’s Up with the Moon? – 9 (Back to top) PhotoBlogs – 11 1 Stargazers’ Diary – 15 May 2011 Sunday Monday Tuesday Wednesday Thursday Friday Saturday 1 2 3 4 5 6 7 New Moon Museum 1:51 am Star Party Lunation 1093 3 R F Star Party Fort Worth: New Moon Moonrise 9:58 am Weekend Illuminated: 20.4% 8 9 10 11 12 13 14 First Qtr Moon 3 R F 3:33 pm Lunar Party Werner X Low in West & barely visible to us this month. (Peaks Challenge binary star for May: 48 Virginis @ 11:24 pm – shortly Notable variable star for May: R Hydrae (Hydra) before Moonset) Notable carbon star for May: SS Virginis Fort Worth: Moonset:12:25 am 15 16 17 Full Moon 18 19 20 21 Moon at Perigee 6:09 am 6 am (225,021 miles) FWAS Meeting Exoplanets & the Search for Habitable Worlds Dr. Sara Seager Normal Room 22 23 24 25 26 27 28 Moon at Apogee Last Qtr Moon Algol @ Minima 7:07 am 5 am 9:40 pm NW (251,036 miles) 29 30 31 Top ten deep-sky objects for May: M3, M51, M63, M64, M83, M87, M104, M106, NGC 4449, NGC 4565 Top ten binocular deep-sky objects for May: M3, M51, M63, M64, M84, M86, M87, M104, M106, Mel 111 Challenge deep-sky object for May: 3C 273 (Virgo) (Some objects require dark skies to be seen.) Memorial Day June 2011 Sunday Monday Tuesday Wednesday Thursday Friday Saturday 1 2 3 4 New Moon Museum 4:03 pm Star Party Lunation 1094 3 R F Challenge: Star Party Sunset 8:32 pm Moonset 8:40 pm Can you see the Fort Worth: super-thin crescent Moonrise 8:52 am Moon? New Moon Moonset:11:07 pm You’d better have a high vantage point. -
Lopsided Spiral Galaxies: Evidence for Gas Accretion
A&A 438, 507–520 (2005) Astronomy DOI: 10.1051/0004-6361:20052631 & c ESO 2005 Astrophysics Lopsided spiral galaxies: evidence for gas accretion F. Bournaud1, F. Combes1,C.J.Jog2, and I. Puerari3 1 Observatoire de Paris, LERMA, 61 Av. de l’Observatoire, 75014 Paris, France e-mail: [email protected] 2 Department of Physics, Indian Institute of Science, Bangalore 560012, India 3 Instituto Nacional de Astrofísica, Optica y Electrónica, Calle Luis Enrique Erro 1, 72840 Tonantzintla, Puebla, Mexico Received 3 January 2005 / Accepted 15 March 2005 Abstract. We quantify the degree of lopsidedness for a sample of 149 galaxies observed in the near-infrared from the OSUBGS sample, and try to explain the physical origin of the observed disk lopsidedness. We confirm previous studies, but for a larger sample, that a large fraction of galaxies have significant lopsidedness in their stellar disks, measured as the Fourier amplitude of the m = 1 component normalised to the average or m = 0 component in the surface density. Late-type galaxies are found to be more lopsided, while the presence of m = 2 spiral arms and bars is correlated with disk lopsidedness. We also show that the m = 1 amplitude is uncorrelated with the presence of companions. Numerical simulations were carried out to study the generation of m = 1viadifferent processes: galaxy tidal encounters, galaxy mergers, and external gas accretion with subsequent star formation. These simulations show that galaxy interactions and mergers can trigger strong lopsidedness, but do not explain several independent statistical properties of observed galaxies. To explain all the observational results, it is required that a large fraction of lopsidedness results from cosmological accretion of gas on galactic disks, which can create strongly lopsided disks when this accretion is asymmetrical enough. -
San Jose Astronomical Association Membership Form P.O
SJAA EPHEMERIS SJAA Activities Calendar May General Meeting Jim Van Nuland Dr. Jeffrey Cuzzi May 26 at 8 p.m. @ Houge Park late April David Smith 20 Houge Park Astro Day. Sunset 7:47 p.m., 20% moon sets 0:20 a.m. Star party hours: 8:30 to 11:30 p.m. At our May 26 General Meeting the title of the talk will be: 21 Mirror-making workshop at Houge Park. 7:30 p.m. What Have We Learned from the Cassini/Huygens Mission to 28 General meeting at Houge Park. Karrie Gilbert will Saturn? – a presentation by Dr. Jeffrey Cuzzi of NASA Ames speak on Studies of Andromeda Galaxy Halo Stars. 8 Research Center. p.m. May Cassini is now well into its third year at Saturn. The Huygens 5 Mirror-making workshop at Houge Park. 7:30 p.m. entry probe landed on Titan in January 2005, but since then, 11 Astronomy Class at Houge Park. 7:30 p.m. many new discoveries have been made on Titan’s surface, and 11 Houge Park star party. Sunset 8:06 p.m., 27% moon elsewhere in the system, by the orbiter as it continues its four- rise 3:23 a.m. Star party hours: 9:00 to midnight. year tour. In addition, new understanding is emerging from 12 Dark sky weekend. Sunset 8:07 p.m., 17% moon rise analysis of the earliest obtained data. 3:50 a.m. In this talk, Dr. Jeffrey Cuzzi will review the key science highlights 17 Mirror-making workshop at Houge Park. -
SAC's 110 Best of the NGC
SAC's 110 Best of the NGC by Paul Dickson Version: 1.4 | March 26, 1997 Copyright °c 1996, by Paul Dickson. All rights reserved If you purchased this book from Paul Dickson directly, please ignore this form. I already have most of this information. Why Should You Register This Book? Please register your copy of this book. I have done two book, SAC's 110 Best of the NGC and the Messier Logbook. In the works for late 1997 is a four volume set for the Herschel 400. q I am a beginner and I bought this book to get start with deep-sky observing. q I am an intermediate observer. I bought this book to observe these objects again. q I am an advance observer. I bought this book to add to my collect and/or re-observe these objects again. The book I'm registering is: q SAC's 110 Best of the NGC q Messier Logbook q I would like to purchase a copy of Herschel 400 book when it becomes available. Club Name: __________________________________________ Your Name: __________________________________________ Address: ____________________________________________ City: __________________ State: ____ Zip Code: _________ Mail this to: or E-mail it to: Paul Dickson 7714 N 36th Ave [email protected] Phoenix, AZ 85051-6401 After Observing the Messier Catalog, Try this Observing List: SAC's 110 Best of the NGC [email protected] http://www.seds.org/pub/info/newsletters/sacnews/html/sac.110.best.ngc.html SAC's 110 Best of the NGC is an observing list of some of the best objects after those in the Messier Catalog.