FM 6-300 O Effective 1 January 1983 FIELD MANUAL HEADQUARTERS DEPARTMENT of the ARMY .No

Total Page:16

File Type:pdf, Size:1020Kb

FM 6-300 O Effective 1 January 1983 FIELD MANUAL HEADQUARTERS DEPARTMENT of the ARMY .No F t- %5T> Mfr- (Q)' terence 's û CD o LTL O ☆ <D o run «D O O O [xn * 8 g <ÿ0 n n Æô O O û o< ☆ û G ,0 O û û- ☆ <?û û ☆ ° ûû û d c? ft O "C? "ù O ☆ s> û Ô O ☆ Û t> Cf O £? û, U ébùp û <D OC? Oû o)M p-’l cfJ-) o tS> O O c? O PiSFMUilMîlKîf @ÎF IHSIl MEM¥ «D The ñsm¡f library (ANRAL) ATTM: Mtitkrry Documents loom lASlß, Pentagon M^hingtos« D.Q. \ f SL Í. m Í i i A / *FM 6-300 O Effective 1 January 1983 FIELD MANUAL HEADQUARTERS DEPARTMENT OF THE ARMY .No. 6-300 Washington, DC, 2 October 1982 ARMY EPHEMERIS 1983-1987 Page CHAPTER 1. INTRODUCTION 1-1 CHAPTERX 2. ASTRONOMICAL TABLES AND CHARTS 2-1 Table \a. Astronomic refraction corrected for temperature (degrees) 2-1 16\ Astronomic refraction corrected for temperature (mils) 2-5 ressure correction factor Cb 2-8 2a. Sun, 1983, for zero hours universal time (GMT) . 2-9 2b. Sun\l984, for zero hours universal time (GMT) . 2-21 2c. Sun, \985, for zero hours universal time (GMT) . 2-33 2d Sun, 1986, for zero hours universal time (GMT) . 2-45 2e. Sun, 1987, for zero hours universal time (GMT) . 2-57 3. Equation of time graph 2-69 4. Correction «9 Greenwich mean time interval to obtain Greenwich sidereal time interval 2-70 5a. Conversion of rime to arc 2-72 56. Conversion of arfe to time 2-73 5c. Conversion of decrees, minutes, and seconds to mils 2-74 6. Convergence. 2-75 6a. Grid convergence nomograph 2-88 7. Second term in convergence computation, UTM coordinates 2-89 8a. Second term in converge\ce computation, geographic coordinates (degrees). 2-91 86. Second term in convergencd^computation, geographic coordinates (mils) 2-92 9. Alphabetical star list 2-93 ^0a(1J. Apparent places of stars, 1983 (îtegrees). 2-95 103^2/ Apparent places of stars, 1984 (dé 2-99 10af3/ Apparent places of stars, 1985 (de^ 2-103 103(4). Apparent places of stars, 1986 (deg 2-107 10af'S/ Apparent places of stars, 1987 (degreè 2-111 106(7/ Apparent places of stars, 1983 (mils of\feclination).. 2-115 106(2/ Apparent places of stars, 1984 (mils of dfeclination)... 2-119 10b(3). Apparent places of stars, 1985 (mils of declination)... 2-123 106(4/ Apparent places of stars, 1986 (mils of declination)... 2-127 106(5/ Apparent places of stars, 1987 (mils of declination).. 2-131 11a. Apparent places of Polaris (star no 10), 1983. 2-135 116. Apparent places of Polaris (star no 10), 1984. 2-136 llc. Apparent places of Polaris (star no 10), 1985. 2-137 lld. Apparent places of Polaris (star no 10), 1986. 2-138 lie. Apparent places of Polaris (star no 10), 1987. 2-139 'his manual supersedes FM 6-300, 2 October 1981. FM 6-300 Page 12a. To determine azimuth from Polaris, 1983 2-143 126. To determine azimuth from Polaris, 1984 2-145 12c. To determine azimuth from Polaris, 1985 2-147 12t/. To determine azimuth from Polaris, 1986 2-149 12e. To determine azimuth from Polaris, 1987 2-151 13. Grid azimuth correction, simultaneous observation 2-153 14. Zone-to-zone azimuth transformation 2-154 ii FM 6-300 CHAPTER 1 INTRODUCTION 1 -1. Purpose and Scope Artillery School. The basic astronomical data is furnished by H. M. Nautical Almanac Office, a. This manual is a compilation of tables and Royal Greenwich Observatory, and the Nautical charts for use in computing astronomical Almanac Office, US Naval Observatory. azimuths for the field artillery. These tables and c. Users of this manual are encouraged to charts are used for computing azimuth of the submit recommended changes or comments to Sun or selected stars by either the altitude or improve the manual. Comments should be hour-angle method. Special tables (tables keyed to the specific page, paragraph, and line of 12-12e), which are tabular methods of the text in which the change is recommended. computing Polaris, are included for a rapid Reasons should be provided for each comment computation of a Polaris azimuth. The secant to insure understanding and complete tables accompanying these tables are evaluation. Comments should be prepared permanent. Tables and charts are also included using DA Form 2028 (Recommended Changes to correct astronomic azimuth to grid azimuth, to to Publications and Blank Forms) and forwarded extend azimuth by simultaneous observation, direct to the Commandant, US Army Field and to perform zone-to-zone transformation of Artillery School, ATTN: ATSF-DL, Fort Sill, azimuth. Oklahoma 73503. b. Data contained in tables 2a, 2b, 2c, 2d, 2e, 10a(1), 10a(2), 10a(3), 10a(4), 10a(5), 10b(1), 1 -2. Description of Tables and Charts 10b(2), 10b(3), 10b(4), 10b(5), 11a, 11b, 11c, lid, lie, 12a, 12b, 12c, 12d, and 12e are This manual is intended to be used as a current only for the years in which the manual is companion publication to FM 6-2, Field Artillery effective. These tables are compiled by the Survey. Details on the computation of Counterfire Department, under the supervision astronomical azimuth and the use of these of the NOAA Liaison Officer, US Army Field tables and charts are contained in FM 6-2. 1-1 FM 6-300 CHAPTER 2 ASTRONOMICAL TABLES AND CHARTS Tablela. Astronomic Refraction Corrected for Temperature (Degrees) TO BE SUBTRACTED FROM OBSERVED ALTITUDE OF SUN OR STAR (Use values of observed altitude and temperature nearest the values tabulated as arguments.) Temperature F. Observed altitude -30 -20 -10 0 +10 +20 +30 +40 +50 +60 +70 +80 +90 +100 +110 +120 +130 00 00 40-43 39-45 38-53 384)2 37-15 36-27 36-44 354)1 34-20 33-40 3501 32-26 31-51 31-36 3543 3514 2546 20 35-57 354)6 34-20 33-35 32-53 32-11 31-33 30-55 30-18 29-44 2509 2538 2507 27-37 274)7 2542 2517 40 32-00 31-15 30-34 29-54 29-16 28-39 28-05 27-31 26-59 2528 2557 2530 2502 24-35 244» 2546 2523 01 00 28-42 284)1 27-25 26-49 26-15 25-42 25-12 24-41 24-12 2544 2517 22-52 22-27 22-03 21-40 21-19 2559 20 25-55 25-19 24-46 24-13 23-43 23-13 22-45 22-18 21-61 21-26 21-02 2539 2517 1555 1544 1516 1557 40 23-34 234X) 22-31 224)1 21-33 21-06 20-41 20-16 19-52 1529 1507 1546 1526 1506 17-47 17-30 17-13 02 00 21-32 214)2 20-35 204)7 19-42 19-17 18-54 18-31 18-10 17-49 17-28 17-10 1551 1533 1515 1500 1545 20 19-48 19-20 18-54 18-29 18-06 17-43 17-22 17-01 1541 1522 1503 1546 1529 1512 14-66 14-42 14-28 40 18-17 17-51 17-28 17-05 16-43 16-22 164» 15-43 1525 1507 14-50 14-34 14-18 144)2 1548 1536 1522 03 00 16-57 16-33 16-12 15-50 15-30 15-11 14-53 14-35 14-18 144)1 1545 1530 1516 1501 12-48 12-36 12-24 20 15-47 15-25 154)5 14-45 14-27 144» 13-51 13-35 13-19 1504 12-48 12-35 12-21 124» 11-55 11-44 11-32 40 14-45 14-25 14-06 13-47 13-30 13-13 12-57 12-42 12-27 12-12 11-58 11-46 11-33 11-20 114» 1558 1547 04 00 13-50 13-31 13-13 12-56 12-40 12-24 124)9 11-54 11-40 11-27 11-14 114)2 1550 1538 1527 1517 1507 20 13-01 12-43 12-26 12-10 11-55 11-40 11-26 11-12 10-59 1546 1534 1523 1511 1500 0560 0540 0531 40 12-17 12-00 11-44 11-29 11-14 11-00 10-47 10-34 10-22 1510 0558 0547 0537 0526 0516 0508 0559 05 00 11-38 11-21 114)7 10-52 10-38 10-25 10-13 10-00 09-48 0537 0526 0516 094» 0556 0547 0538 0530 20 11-02 10-46 10-32 10-18 10-05 09-53 09-41 09-29 09-18 0507 0557 0547 0538 0528 0519 0512 0504 40 10-29 10-14 10-01 09-48 09-35 09-23 09-12 094)1 08-50 0540 0530 0521 0512 0503 07-55 07-47 07-40 06 00 09-59 09-45 09-32 09-20 094» 08-56 08-46 08-35 08-25 0516 0506 07-57 07-49 07-40 07-32 07-25 07-18 20 09-32 09-18 09-06 08-54 08-43 08-32 08-22 08-12 084)2 07-53 07-44 07-35 07-27 07-19 07-11 074» 0558 40 094)7 08-54 08-42 08-31 08-20 08-09 084)0 07-50 07-41 07-32 07-23 07-16 074» 074» 0553 0546 0540 07 00 08-43 08-31 08-20 08-09 07-59 07-49 07-39 07-30 07-21 07-13 074» 0557 0550 0542 0535 0529 0523 20 08-22 08-10 08-00 07-49 07-39 07-30 07-21 07-12 07-03 0555 0547 0540 0533 0526 0519 0513 0507 40 084)2 07-51 07-41 07-31 07-21 07-12 07-03 06-55 0547 0539 0531 0524 0517 0510 0504 0558 0553 08 00 07-44 07-33 07-23 07-13 07-04 06-55 06-47 06-39 0531 0524 0516 0510 0503 0556 0560 0545 0539 20 07-27 07-16 07-07 06-57 06-49 06-40 06-32 06-24 0517 0509 0502 0556 0549 0543 0537 0532 0527 40 07-11 07-01 06-52 06-42 06-34 06-26 06-18 06-10 0503 0556 0549 0543 0537 0531 0525 0520 0515 09 00 06-56 06-46 06-37 06-28 06-20 06-12 06-05 05-58 0551 0544 0537 0531 0525 0519 0514 0509 0504 20 06-42 06-32 06-24 06-15 06-08 064X) 05-53 05-46 0539 0532 0526 0520 0514 054» 0503 04-58 04-54 40 06-29 06-19 06-11 06-03 05-56 05-48 05-41 0534 0528 0521 0515 0510 0504 04-59 04-53 04-49 04-44 10 00 06-16 06-07 06-00 05-52 05-44 05-37 05-30 0524 0517 0511 0505 0500 04-54 04-49 04-44 04-40 04-35.
Recommended publications
  • 1989Aj 97. . 51 Om the Astronomical Journal Volume 97, Number 2 February 1989 Iccd Speckle Observations of Binary Stars. Iv
    OM 51 . THE ASTRONOMICAL JOURNAL VOLUME 97, NUMBER 2 FEBRUARY 1989 97. ICCD SPECKLE OBSERVATIONS OF BINARY STARS. IV. MEASUREMENTS DURING 1986-1988 FROM THE KITT PEAK 4 m TELESCOPE Harold A. McAlister,a) William I. Hartkopf,a) James R. Sowell,10 1989AJ and Edmund G. Dombrowski“’ Center for High Angular Resolution Astronomy, Georgia State University, Atlanta, Georgia 30303 OttoG. Franz3) Lowell Observatory, Flagstaff, Arizona 86001 Received 29 August 1988; revised 12 October 1988 ABSTRACT One thousand five hundred and fifty measurements of 1006 binary star systems observed mostly during 1986 through mid-1988 by means of speckle interferometry with the KPNO 4 m telescope are present- ed. Twenty-one systems are directly resolved for the first time, including new components to the cool supergiant a Her A and the Pleiades shell star Pleione. A continuing survey of The Bright Star Cata- logue yielded eight new binaries from 293 bright stars observed. Corrections to speckle measures from the GSU/CHARA ICCD speckle camera previously published are presented and discussed. I. INTRODUCTION for the 1983-1984 data is due to the somewhat lower quality This paper presents further results from a continuing pro- of the calibration data available for that particular time peri- gram of binary star speckle interferometry carried out at the od. We now adopt a calibration based upon the mean of all 4 m Mayall telescope at Kitt Peak National Observatory. A the scale and orientation measurements that we have deter- detailed description of the observational technique and in- mined since the initiation of our ICCD speckle-camera sys- strumentation, and of the methods of data reduction, analy- tem.
    [Show full text]
  • JOHN R. THORSTENSEN Address
    CURRICULUM VITAE: JOHN R. THORSTENSEN Address: Department of Physics and Astronomy Dartmouth College 6127 Wilder Laboratory Hanover, NH 03755-3528; (603)-646-2869 [email protected] Undergraduate Studies: Haverford College, B. A. 1974 Astronomy and Physics double major, High Honors in both. Graduate Studies: Ph. D., 1980, University of California, Berkeley Astronomy Department Dissertation : \Optical Studies of Faint Blue X-ray Stars" Graduate Advisor: Professor C. Stuart Bowyer Employment History: Department of Physics and Astronomy, Dartmouth College: { Professor, July 1991 { present { Associate Professor, July 1986 { July 1991 { Assistant Professor, September 1980 { June 1986 Research Assistant, Space Sciences Lab., U.C. Berkeley, 1975 { 1980. Summer Student, National Radio Astronomy Observatory, 1974. Summer Student, Bartol Research Foundation, 1973. Consultant, IBM Corporation, 1973. (STARMAP program). Honors and Awards: Phi Beta Kappa, 1974. National Science Foundation Graduate Fellow, 1974 { 1977. Dorothea Klumpke Roberts Award of the Berkeley Astronomy Dept., 1978. Professional Societies: American Astronomical Society Astronomical Society of the Pacific International Astronomical Union Lifetime Publication List * \Can Collapsed Stars Close the Universe?" Thorstensen, J. R., and Partridge, R. B. 1975, Ap. J., 200, 527. \Optical Identification of Nova Scuti 1975." Raff, M. I., and Thorstensen, J. 1975, P. A. S. P., 87, 593. \Photometry of Slow X-ray Pulsars II: The 13.9 Minute Period of X Persei." Margon, B., Thorstensen, J., Bowyer, S., Mason, K. O., White, N. E., Sanford, P. W., Parkes, G., Stone, R. P. S., and Bailey, J. 1977, Ap. J., 218, 504. \A Spectrophotometric Survey of the A 0535+26 Field." Margon, B., Thorstensen, J., Nelson, J., Chanan, G., and Bowyer, S.
    [Show full text]
  • Annual Report 2016–2017 AAVSO
    AAVSO The American Association of Variable Star Observers Annual Report 2016–2017 AAVSO Annual Report 2012 –2013 The American Association of Variable Star Observers AAVSO Annual Report 2016–2017 The American Association of Variable Star Observers 49 Bay State Road Cambridge, MA 02138-1203 USA Telephone: 617-354-0484 Fax: 617-354-0665 email: [email protected] website: https://www.aavso.org Annual Report Website: https://www.aavso.org/annual-report On the cover... At the 2017 AAVSO Annual Meeting.(clockwise from upper left) Knicole Colon, Koji Mukai, Dennis Conti, Kristine Larsen, Joey Rodriguez; Rachid El Hamri, Andy Block, Jane Glanzer, Erin Aadland, Jamin Welch, Stella Kafka; and (clockwise from upper left) Joey Rodriguez, Knicole Colon, Koji Mukai, Frans-Josef “Josch” Hambsch, Chandler Barnes. Picture credits In additon to images from the AAVSO and its archives, the editors gratefully acknowledge the following for their image contributions: Glenn Chaple, Shawn Dvorak, Mary Glennon, Bill Goff, Barbara Harris, Mario Motta, NASA, Gary Poyner, Msgr. Ronald Royer, the Mary Lea Shane Archives of the Lick Observatory, Chris Stephan, and Wheatley, et al. 2003, MNRAS, 345, 49. Table of Contents 1. About the AAVSO Vision and Mission Statement 1 About the AAVSO 1 What We Do 2 What Are Variable Stars? 3 Why Observe Variable Stars? 3 The AAVSO International Database 4 Observing Variable Stars 6 Services to Astronomy 7 Education and Outreach 9 2. The Year in Review Introduction 11 The 106th AAVSO Spring Membership Meeting, Ontario, California 11 The
    [Show full text]
  • National Observatories
    Sidney C Wolff NOAO/DIR NATIONAL OPTICAL ASTRONOMY OBSERVATORIES NATIONAL OPTICAL ASTRONOMY OBSERVATORIES Cerro Tololo Inter-American Observatory Kitt Peak National Observatory National Solar Observatory La Serena, Chile Tucson, Arizona 85726 Sunspot, New Mexico 88349 ANNUAL REPORT October 1996 - September 1997 October 30,1997 TABLE OF CONTENTS L INTRODUCTION IL AURA BOARD m. SCffiNTDJIC PROGRAM A. Cerro Tololo Inter-American Observatory (CTIO) 1. The Search for High Z Supernovae 2. Nearby Stars and Planets 2 B. Kitt Peak National Observatory (KPNO) 3 1. The History of Star Formation in Distant Galaxies 3 2. Oxygen Abundance and the Age of the Universe 4 3. The Age of Elliptical Galaxies - Is There Enough Time? 5 C. National Solar Observatory (NSO) 5 1. Results from GONG 5 2. High-Resolution Images of Solar Magnetic Fields 6 3. Active Optics Control Loop Closed at the Sac Peak Vacuum Tower Telescope 7 IV. DIVISION OPERATIONS 7 A. CTIO 7 Telescope Upgrades and Instrumentation 7 1. 4-m Upgrades 8 2. Major Instrumentation Efforts 9 3. SOAR 4-m Telescope Project 9 4. CCD Implementation and ARCON Controller Development 10 5. Existing Small General-User Telescopes on Cerro Tololo 10 6. New "Tenant" Installations and Upgrades 10 7. Other 11 B. KPNO 12 1. Image Quality Improvements 12 2. WTYN Queue Observing Experiment 12 3. WTYN 13 4. KPNO Instrumentation Improvements 14 5. Burrell-Schmidt 14 C. NSO 15 1. Kitt Peak 15 2. Sacramento Peak 17 3. Digital Library Development 21 D. USGP/ScOpe 21 E. NOAO Instrumentation 25 1. CCD Mosaic Imager 26 2.
    [Show full text]
  • LIST of PUBLICATIONS Aryabhatta Research Institute of Observational Sciences ARIES (An Autonomous Scientific Research Institute
    LIST OF PUBLICATIONS Aryabhatta Research Institute of Observational Sciences ARIES (An Autonomous Scientific Research Institute of Department of Science and Technology, Govt. of India) Manora Peak, Naini Tal - 263 129, India (1955−2020) ABBREVIATIONS AA: Astronomy and Astrophysics AASS: Astronomy and Astrophysics Supplement Series ACTA: Acta Astronomica AJ: Astronomical Journal ANG: Annals de Geophysique Ap. J.: Astrophysical Journal ASP: Astronomical Society of Pacific ASR: Advances in Space Research ASS: Astrophysics and Space Science AE: Atmospheric Environment ASL: Atmospheric Science Letters BA: Baltic Astronomy BAC: Bulletin Astronomical Institute of Czechoslovakia BASI: Bulletin of the Astronomical Society of India BIVS: Bulletin of the Indian Vacuum Society BNIS: Bulletin of National Institute of Sciences CJAA: Chinese Journal of Astronomy and Astrophysics CS: Current Science EPS: Earth Planets Space GRL : Geophysical Research Letters IAU: International Astronomical Union IBVS: Information Bulletin on Variable Stars IJHS: Indian Journal of History of Science IJPAP: Indian Journal of Pure and Applied Physics IJRSP: Indian Journal of Radio and Space Physics INSA: Indian National Science Academy JAA: Journal of Astrophysics and Astronomy JAMC: Journal of Applied Meterology and Climatology JATP: Journal of Atmospheric and Terrestrial Physics JBAA: Journal of British Astronomical Association JCAP: Journal of Cosmology and Astroparticle Physics JESS : Jr. of Earth System Science JGR : Journal of Geophysical Research JIGR: Journal of Indian
    [Show full text]
  • GEORGE HERBIG and Early Stellar Evolution
    GEORGE HERBIG and Early Stellar Evolution Bo Reipurth Institute for Astronomy Special Publications No. 1 George Herbig in 1960 —————————————————————– GEORGE HERBIG and Early Stellar Evolution —————————————————————– Bo Reipurth Institute for Astronomy University of Hawaii at Manoa 640 North Aohoku Place Hilo, HI 96720 USA . Dedicated to Hannelore Herbig c 2016 by Bo Reipurth Version 1.0 – April 19, 2016 Cover Image: The HH 24 complex in the Lynds 1630 cloud in Orion was discov- ered by Herbig and Kuhi in 1963. This near-infrared HST image shows several collimated Herbig-Haro jets emanating from an embedded multiple system of T Tauri stars. Courtesy Space Telescope Science Institute. This book can be referenced as follows: Reipurth, B. 2016, http://ifa.hawaii.edu/SP1 i FOREWORD I first learned about George Herbig’s work when I was a teenager. I grew up in Denmark in the 1950s, a time when Europe was healing the wounds after the ravages of the Second World War. Already at the age of 7 I had fallen in love with astronomy, but information was very hard to come by in those days, so I scraped together what I could, mainly relying on the local library. At some point I was introduced to the magazine Sky and Telescope, and soon invested my pocket money in a subscription. Every month I would sit at our dining room table with a dictionary and work my way through the latest issue. In one issue I read about Herbig-Haro objects, and I was completely mesmerized that these objects could be signposts of the formation of stars, and I dreamt about some day being able to contribute to this field of study.
    [Show full text]
  • The Handbook of the British Astronomical Association
    THE HANDBOOK OF THE BRITISH ASTRONOMICAL ASSOCIATION 2012 Saturn’s great white spot of 2011 2011 October ISSN 0068-130-X CONTENTS CALENDAR 2012 . 2 PREFACE. 3 HIGHLIGHTS FOR 2012. 4 SKY DIARY . .. 5 VISIBILITY OF PLANETS. 6 RISING AND SETTING OF THE PLANETS IN LATITUDES 52°N AND 35°S. 7-8 ECLIPSES . 9-15 TIME. 16-17 EARTH AND SUN. 18-20 MOON . 21 SUN’S SELENOGRAPHIC COLONGITUDE. 22 MOONRISE AND MOONSET . 23-27 LUNAR OCCULTATIONS . 28-34 GRAZING LUNAR OCCULTATIONS. 35-36 PLANETS – EXPLANATION OF TABLES. 37 APPEARANCE OF PLANETS. 38 MERCURY. 39-40 VENUS. 41 MARS. 42-43 ASTEROIDS AND DWARF PLANETS. 44-60 JUPITER . 61-64 SATELLITES OF JUPITER . 65-79 SATURN. 80-83 SATELLITES OF SATURN . 84-87 URANUS. 88 NEPTUNE. 89 COMETS. 90-96 METEOR DIARY . 97-99 VARIABLE STARS . 100-105 Algol; λ Tauri; RZ Cassiopeiae; Mira Stars; eta Geminorum EPHEMERIDES OF DOUBLE STARS . 106-107 BRIGHT STARS . 108 ACTIVE GALAXIES . 109 INTERNET RESOURCES. 110-111 GREEK ALPHABET. 111 ERRATA . 112 Front Cover: Saturn’s great white spot of 2011: Image taken on 2011 March 21 00:10 UT by Damian Peach using a 356mm reflector and PGR Flea3 camera from Selsey, UK. Processed with Registax and Photoshop. British Astronomical Association HANDBOOK FOR 2012 NINETY-FIRST YEAR OF PUBLICATION BURLINGTON HOUSE, PICCADILLY, LONDON, W1J 0DU Telephone 020 7734 4145 2 CALENDAR 2012 January February March April May June July August September October November December Day Day Day Day Day Day Day Day Day Day Day Day Day Day Day Day Day Day Day Day Day Day Day Day Day of of of of of of of of of of of of of of of of of of of of of of of of of Month Week Year Week Year Week Year Week Year Week Year Week Year Week Year Week Year Week Year Week Year Week Year Week Year 1 Sun.
    [Show full text]
  • A Common Proper Motion Companion to the Exoplanet Host 51 Pegasi 4 John Greaves
    University of South Alabama Journal of Double Star Observations VOLUME 2 NUMBER 1 WINTER 2006 We have lots of great articles in this issue including new measurements from the Dave Arnold and an article from Brian Mason describing data files from the USNO. We also have an article about the Aitken criterion from Francisco Rica Romero. Robert G. Aitken (1864—1951) was the grand old man of double star astronomy and still observed doubles visually long http://www.phys-astro.sonoma.edu after others had turned to photography. He ranks sixth on the list of double star observations, was on the board of directors of the Astronomical Society of the Pacific for decades, author of the wonderful book The Binary Stars, and was hearing impaired. Check out Rica Romero's article on page 36. NEW WEB ADDRESS The JDSO now has a new web address. You must have learned that by now or you wouldn't be reading this! Anyway, we knew that our old url was very awkward and inappropriate, so we acquired www.jdso.org. If you forget and go to our old address by mistake, that's OK, you will be transferred to the new address automatically. Robert Grant Aitken Thanks for looking us up! Inside this issue: Is HLD 32 A (= WDS 18028-2705 A) an Unresolved Binary Candidate? 2 Francisco M. Rica Romero A Common Proper Motion Companion to the Exoplanet Host 51 Pegasi 4 John Greaves Divinus Lux Observatory Bulletin: Report #1 6 Dave Arnold Divinus Lux Observatory Bulletin: Report #2 13 Dave Arnold Requested Double Star Data from the U.S.
    [Show full text]
  • Binary Star Speckle Measurements at Calar Alto. I
    A&A 366, 868–872 (2001) Astronomy DOI: 10.1051/0004-6361:20000298 & c ESO 2001 Astrophysics Binary star speckle measurements at Calar Alto. I. J. A. Docobo1,V.S.Tamazian1, Yu. Yu. Balega2,J.Blanco1,A.F.Maximov2, and V. A. Vasyuk2 1 Astronomical Observatory Ramon Maria Aller, University of Santiago de Compostela. PO Box 197, Santiago de Compostela, Spain 2 Special Astrophysical Observatory, Zelenchuk region, 369167, Russia Received 24 May 2000 / Accepted 14 November 2000 Abstract. We present the first results of our speckle interferometric measurements of binary stars made with the ICCD speckle camera using the 1.52-m telescope of the Observatorio Astronomico Nacional at Calar Alto (Spain) in September, 1999. The data contain 123 observations of 83 systems. The measured angular separations range from 000. 153 to 600. 727. We have used there new speckle measurements to improve the orbital elements for the binaries COU 247 and BU 524 AB. Key words. binaries: visual – interferometry 1. Introduction Russian Academy of Sciences. The new instrument has been used for speckle observations of binary stars using At the present time, although the orbits for more than the 1.52-m telescope at Calar Alto, in 1999. Below, we 1000 visual binaries are available, the study of orbital mo- provide a brief description of the instrument and report tion of visual and interferometric pairs remains an impor- on the first interferometric data obtained. Orbits of visual tant astronomical discipline. Visual binaries are the key binaries Cou 247 and Bu 524 were improved using the new source of information about stellar masses and distances, measurements.
    [Show full text]
  • Measurements in 1998 M
    Speckle observations of double stars with PISCO at Pic du Midi: measurements in 1998 M. Scardia, Jean-Louis Prieur, Eric Aristidi, L. Koechlin To cite this version: M. Scardia, Jean-Louis Prieur, Eric Aristidi, L. Koechlin. Speckle observations of double stars with PISCO at Pic du Midi: measurements in 1998. Astrophysical Journal Supplement, American Astro- nomical Society, 2000, 131, pp.561-569. hal-02443006 HAL Id: hal-02443006 https://hal.archives-ouvertes.fr/hal-02443006 Submitted on 16 Jan 2020 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. Speckle observations of double stars with PISCO at Pic du Midi: measurements in 1998. Scardia, M. Osservatorio Astronomico di Brera, Via E. Bianchi 46, 22055 Merate, Italy and Prieur, J.-L. UMR 5572 d’Astrophysique, Observatoire Midi-Pyr´en´ees – Centre National de la Recherche Scientifique, 14, Avenue Edouard Belin, 31400 Toulouse, France and Aristidi, E. UMR 6525 Astrophysique, Universit´ede Nice Sophia - Antipolis – Centre National de la Recherche Scientifique, Parc Valrose, 06108 Nice Cedex 2, France and Koechlin, L. UMR 5572 d’Astrophysique, Observatoire Midi-Pyr´en´ees – Centre National de la Recherche Scientifique, 14, Avenue Edouard Belin, 31400 Toulouse, France ABSTRACT We present astrometric measurements of binary stars based on speckle observations of 164 in- dependent sequences of observations (∼ 104 frames each) made with the PISCO speckle camera at Pic du Midi.
    [Show full text]
  • Company Vendor ID (Decimal Format) (AVL) Ditest Fahrzeugdiagnose Gmbh 4621 @Pos.Com 3765 0XF8 Limited 10737 1MORE INC
    Vendor ID Company (Decimal Format) (AVL) DiTEST Fahrzeugdiagnose GmbH 4621 @pos.com 3765 0XF8 Limited 10737 1MORE INC. 12048 360fly, Inc. 11161 3C TEK CORP. 9397 3D Imaging & Simulations Corp. (3DISC) 11190 3D Systems Corporation 10632 3DRUDDER 11770 3eYamaichi Electronics Co., Ltd. 8709 3M Cogent, Inc. 7717 3M Scott 8463 3T B.V. 11721 4iiii Innovations Inc. 10009 4Links Limited 10728 4MOD Technology 10244 64seconds, Inc. 12215 77 Elektronika Kft. 11175 89 North, Inc. 12070 Shenzhen 8Bitdo Tech Co., Ltd. 11720 90meter Solutions, Inc. 12086 A‐FOUR TECH CO., LTD. 2522 A‐One Co., Ltd. 10116 A‐Tec Subsystem, Inc. 2164 A‐VEKT K.K. 11459 A. Eberle GmbH & Co. KG 6910 a.tron3d GmbH 9965 A&T Corporation 11849 Aaronia AG 12146 abatec group AG 10371 ABB India Limited 11250 ABILITY ENTERPRISE CO., LTD. 5145 Abionic SA 12412 AbleNet Inc. 8262 Ableton AG 10626 ABOV Semiconductor Co., Ltd. 6697 Absolute USA 10972 AcBel Polytech Inc. 12335 Access Network Technology Limited 10568 ACCUCOMM, INC. 10219 Accumetrics Associates, Inc. 10392 Accusys, Inc. 5055 Ace Karaoke Corp. 8799 ACELLA 8758 Acer, Inc. 1282 Aces Electronics Co., Ltd. 7347 Aclima Inc. 10273 ACON, Advanced‐Connectek, Inc. 1314 Acoustic Arc Technology Holding Limited 12353 ACR Braendli & Voegeli AG 11152 Acromag Inc. 9855 Acroname Inc. 9471 Action Industries (M) SDN BHD 11715 Action Star Technology Co., Ltd. 2101 Actions Microelectronics Co., Ltd. 7649 Actions Semiconductor Co., Ltd. 4310 Active Mind Technology 10505 Qorvo, Inc 11744 Activision 5168 Acute Technology Inc. 10876 Adam Tech 5437 Adapt‐IP Company 10990 Adaptertek Technology Co., Ltd. 11329 ADATA Technology Co., Ltd.
    [Show full text]
  • On Hot and Cool Stars, Spectroscopic Investigations in the Ultraviolet
    STELLINGEN BEHOREND BIJ HET PROEFSCHRIFT "ON HOT ÄND COOL STARS, SPECTROSCOPIC INVESTIGATIONS IN THE ULTRAVIOLET" Enkele brede emissielijnen in de spektra van Wolf-Rayet sterren, zoals He II A4686 en C IV A2530 , hebben profielen met versterkte rode vleugels. Dit wijst op de invloed van elektronenverstrooiing op de lijnprofielen in de expanderende WR atmosferen, het zogenaamde Auer-Var. Blerkom effekt. 1J K.A. van der Hucht, H.J. Lamers: 1973, Astrophys. J. 181, 537. 2) L. Auer, D. van Blerkom: 1972, Astrophys. J. 178, 17S. II De argumenten die Conti aanvoert tegen de klassifikatie door Henize et al. 2) van de WN7 ster HD 92740 als dubbelster, gelden eveneens voor de WN7 sterren HD 93131 en HD 151932. P.S. Conti: 1976, Hém. Soa. Foy. des Sei. de Liège, 6e série, tome IX, p. 193. 2) K.G. Henize, J.D. Wray, S.B. Parsons, G.F. Benedict: 1975, Astrophys. J. (Letters) 199, L173. III Een opvallend waarnemingsgegeven is de afwezigheid van H-type superreuzen zwaarder dan ^ 25 MQ. Dit kan verklaard worden door aan te nemen dat, tijdens de overgang van massievere sterren (> 30 Mg^ naar het rode super- reuzenstadium, een zeer hoog massaverlies optreedt. Hierdoor komt het inwendige van zulk een ster tot vlak bij de brandende waterstofschil bloot te liggen. Een zeer hete ster, bijvoorbeeld een Wolf-Rayet ster, blijft dan over. 1) G.S. Bisnovatyi-Kogan, D.K. Nadyozhin: 1972, Astrophys. Space Sei. 15, 353. IV De aanwezigheid van stof rondom een aantal gele superreuzen, suggereert dat deze sterren het rode superreuzenstadium gepasseerd zijn en weer naar links bewegen in het Hertzsprung-Russell diagram.
    [Show full text]