DOCSLIB.ORG

CIRCULAR No. 158 (FEBRUARY 2006)

Total Page：16

File Type：pdf, Size：1020Kb

Download full-text PDF Read full-text
CIRCULAR No. 158 (FEBRUARY 2006) INTERNATIONAL ASTRONOMICAL UNION COMMISSION 26 (DOUBLE STARS) INFORMATION CIRCULAR No. 158 (FEBRUARY 2006) NEW ORBITS ADS Name P T e Ω(2000) 2006 Author(s) α2000δ n a i ω Last ob. 2007 463 HO 3 64y53 1984.84 0.290 116◦5 169◦5 0′′205 CVETKOVIC 00335+4006 5.5784 0′′388 111◦6 143◦1 1996.691 163.1 0.225 684 BU 232 AB 200.96 1914.52 0.621 64.9 250.5 0.85 SCARDIA 00504+5038 1.7914 0.531 31.9 11.4 2006.025 250.9 0.86 et al. (*) 836 A 2901 1517.34 1950.56 0.621 48.4 60.6 0.409 NOVAKOVIC 01015+6922 0.2373 0.990 69.3 330.2 2001.8352 61.0 0.408 1345 A 1 357.02 2205.28 0.299 76.1 249.7 0.818 NOVAKOVIC 01424-0645 1.0083 0.641 50.8 1.9 2003.9600 250.1 0.819 1380 STF 148 625.27 2013.18 0.689 147.9 242.3 0.136 NOVAKOVIC 01461+6349 0.5757 1.081 67.6 121.6 1997.03 252.3 0.137 1729 A 2013 34.66 2005.69 0.593 91.8 282.7 0.130 DOCOBO & 02159+0638 10.3866 0.346 112.3 137.6 2004.9904 265.8 0.165 TAMAZIAN 2799 STT 65 61.00 1998.39 0.635 27.3 183.1 0.087 DOCOBO 03503+2535 5.9016 0.411 84.3 340.5 2004.9906 190.0 0.127 & LING GLE 1 480. 1990.90 0.630 92.3 184.4 0.329 DOCOBO 04163-6057 0.7500 0.890 34.1 35.4 2001.8923 187.8 0.336 & LING 3326 A 1840 AB 128.58 2003.60 0.551 62.4 332.5 0.071 CVETKOVIC 04362+0814 2.7998 0.222 133.0 62.8 1996.869 317.5 0.075 RST 3401 159.41 1966.85 0.473 96.2 273.6 0.420 NOVAKOVIC 04374-0951 2.2583 0.354 143.3 46.2 1991.25 272.5 0.424 3434 HU 612 309.87 1903.76 0.424 3.8 357.6 0.652 NOVAKOVIC 04478+5318 1.1618 0.502 40.3 200.9 2004.924 358.1 0.655 1 NEW ORBITS (continuation) ADS Name P T e Ω(2000) 2006 Author(s) α2000δ n a i ω Last ob. 2007 4020 A 848 534.41 2425.78 0.315 19.8 174.5 0.295 NOVAKOVIC 05255-0033 0.6736 0.400 66.3 17.2 2002.136 175.0 0.298 4229 BU 1240 AB 52.74 1974.93 0.653 127.1 333.9 0.207 RICA 05386+3030 6.8266 0.154 124.2 309.1 2004.095 332.3 0.209 4376 STF 3115 976.83 2131.60 0.338 48.8 338.6 0.790 NOVAKOVIC 05491+6248 0.3685 1.350 131.8 159.4 2003.12 337.9 0.787 5296 STF 945 2679.33 4486.86 0.534 67.4 328.9 0.471 NOVAKOVIC 06404+4058 0.1344 2.307 72.1 186.7 2002.19 329.7 0.471 5726 A 1959 31.85 1988.36 0.008 172.3 166.3 0.255 DOCOBO & 07036+3941 11.3030 0.259 63.3 147.7 2004.9911 171.4 0.261 TAMAZIAN 6381 STF 1146 570.44 2054.74 0.610 12.5 347.4 1.231 NOVAKOVIC 07479-1212 0.6311 2.409 113.9 149.9 2003.253 346.6 1.200 6825 A 550 21.23 1981.30 0.866 71.6 195.9 0.111 CVETKOVIC 08277-0425 16.9589 0.099 149.6 82.1 1996.867 190.8 0.125 COU 1897 165.00 1985.80 0.334 168.1 241.3 0.107 DOCOBO & 08585+3548 2.1818 0.255 61.1 2.3 2004.9911 247.0 0.106 TAMAZIAN COU 1569 117.00 1997.78 0.494 60.7 253.0 0.135 DOCOBO & 10059+3412 3.0769 0.237 69.3 140.1 2004.9913 255.9 0.133 TAMAZIAN 7730 STF 1426 AB 2208.98 2011.15 0.484 127.0 310.3 0.921 NOVAKOVIC 10205+0626 0.1630 1.794 61.1 189.4 2004.304 310.5 0.920 FIN 367 Aa 116.27 2052.18 0.470 155.0 6.1 0.197 MANTE 12064-6543 3.0963 0.222 112.4 286.8 1993.0930 4.8 0.201 9744 HU 580 AB 21.97 2006.98 0.084 70.3 260.7 0.106 DOCOBO 15416+1940 16.3860 0.210 83.2 256.3 2001.5591 276.9 0.050 & LING 11524 HU 198 877.14 2020.98 0.446 130.1 131.0 0.462 NOVAKOVIC 18384+0850 0.4104 0.822 103.7 14.1 2004.2073 130.7 0.461 11956 STF 2437 804.60 2132.95 0.478 114.9 11.4 0.58 SCARDIA 19019+1910 0.4474 0.910 131.0 212.1 2005.662 10.8 0.58 et al. (*) 2 NEW ORBITS (continuation) ADS Name P T e Ω(2000) 2006 Author(s) α2000δ n a i ω Last ob. 2007 LAB 6 Aa 83. 1997.99 0.732 46.4 44.2 0.123 ANDRADE 21287+7034 4.3374 0.195 87.3 194.6 1998.777 44.5 0.140 16731 STT 495 300. 1935.2 0.980 138.6 121.6 0.364 ALZNER 23241+5732 1.2000 0.296 71.0 142.4 2005.80 121.7 0.367 (*) SCARDIA, PRIEUR, PANSECCHI, ARGYLE & BASSO 3 PAPERS PUBLISHED IN 2005 1. ABT, H. A.: Observed Orbital Eccentricities. Astrophys. J. 629 (1), 507 (2005). 2. ALZNER, A.: Micrometer Measurements from 2002.97 to 2004.94. The Webb Soc. Double Star Section Cir. 13, 6 (2005). 3. ANCONELLI, B. et al.: Restoration of interferometric images - IV. An algorithm for super-resolution of stellar systems. Astron. Astrophys. 431 (2), 747 (2005). 4. ARGYLE, R.: Micrometer Measurements from 2004.0 to 2005.0. The Webb Soc. Double Star Section Cir. 13, 1 (2005). 5. BAKIS, V. et al.: Astrometric Solution of the Multiple System Xy Leo. Astrophys. Space Science 296 (1-4), 131. (2005). 6. BALEGA, I. I. et al.: Orbits of new Hipparcos binaries. I. Astron. Astrophys. 433 (2), 591 (2005). 7. BALEGA, Y. Y.; LEUSHIN, V. V. & WEIGELT, G.: Atmospheric Elemental Abun- dances for the Components of the Multiple System ADS 11061. 41 Draconis. Astron. Reports 49 (3), 217 (2005) 8. BALEGA, Y. Y.; LEUSHIN, V. V. & KUZNETSOV, M. K: Atmospheric Chemical Abundances of the Components of the Quadruple System ADS 11061. 40 Draconis. Astron. Reports 49 (12), 984 (2005) 9. BODEN, A. F.; TORRES, G. & HUMMEL, C. A.: Testing Stellar Models with an Improved Physical Orbit for 12 Bootis. Astrophys. J. 627 (1), 464 (2005). 10. BODEN, A. F. et al.: Dynamical Masses for Low-Mass PreMain-Sequence Stars: A Preliminary Physical Orbit for HD 98800 B. Astrophys. J. 635 (1), 442 (2005). 11. BONNELL, I. A. & BATE, M. R.: Binary systems and stellar mergers in massive star formation . Monthly Notices 362 (3), 915 (2005) 12. BOUY, H. et al.: A possible third component in the L dwarf binary system DENIS-P J020529.0-115925 discovered with the HUBBLE space telescope. Astron. J. 129 (1), 511 (2005). 13. BRANHAM, R. L.: Calculating the Apparent Orbit of a Double Star. Astrophys. J. 622 (1), 613 (2005). 14. CARQUILLAT, J.-M.; PRIEUR, J.-L. & UDRY, S.: Contribution to the study of F-G-K-M binaries. X. HD 54901, HD 120544 and HD 123280, three nearby F-type spectroscopic binaries. Astron. Nach. 326 (1), 31 (2005). 15. CARQUILLAT, J.-M.; PRIEUR, J.-L. & GINESTET, N.: Contribution to the study of composite spectra X. HD 3210/1, 27395, 39847, 70826 and 218257/8: five new spectroscopic binaries in multiple systems. Monthly Notices 360 (2), 718 (2005) 4 16. DAVIS, J. et al.: Orbital parameters, masses and distance to β Centauri determined with the Sydney University Stellar Interferometer and high-resolution spectroscopy. Monthly Notices 356 (4), 1362 (2005) 17. FEKEL. F. C. & W. HENRY, G. W.: Chromospherically active stars. XXIV. The giant single-lined binaries HD 37824, HD 181809, and HD 217188. Astron. J. 129 (3), 1669 (2005). 18. FEKEL. F. C. et al.: HD 166181 = V815 Herculis, a single-lined spectroscopic multiple system. Astron. J. 129 (2), 1001 (2005). 19. FRASCA, A. & LANZA, A. F.: Orbital period variation in close binaries from radial velocity data and magnetic activity cycles - II. HR 1099. Astron. Astrophys. 429 (1), 309 (2005). 20. GATEWOOD, G.: An astrometric study of the binary star α Ophiuchi. Astron. J. 130 (2), 809 (2005). 21. GRIFFIN, R. F.: Spectroscopic Binary Orbits from Photoelectric Radial Velocities - Paper 180: Zeta Aurigae. The Observatory 125, 1 (2005). 22. GRIFFIN, R. F.: Spectroscopic Binary Orbits from Photoelectric Radial Velocities - Paper 181: HD 49635/6, HD 50730/1, HD 201563, and HD 203340 . The Obser- vatory 125, 81 (2005). 23. GRIFFIN, R. F.: Spectroscopic Binary Orbits from Photoelectric Radial Velocities - Paper 182: 22 Camelopardalis, HD 156051, HR 6890, and HD221757 . The Observatory 125, 134 (2005). 24. GRIFFIN, R. F.: Spectroscopic Binary Orbits from Photoelectric Radial Velocities - Paper 183: HD 98031, HD 112573, and HD197913 . The Observatory 125, 253 (2005). 25. GRIFFIN, R. F.: Spectroscopic Binary Orbits from Photoelectric Radial Velocities - Paper 184: HD 106383, HD 109070, HD 118157, and HD 121213 . The Observatory 125, 300 (2005). 26. GRIFFIN, R.
Load more

Recommended publications
  • Durham E-Theses
    Durham E-Theses First visibility of the lunar crescent and other problems in historical astronomy. Fatoohi, Louay J. How to cite: Fatoohi, Louay J. (1998) First visibility of the lunar crescent and other problems in historical astronomy., Durham theses, Durham University. Available at Durham E-Theses Online: http://etheses.dur.ac.uk/996/ Use policy The full-text may be used and/or reproduced, and given to third parties in any format or medium, without prior permission or charge, for personal research or study, educational, or not-for-prot purposes provided that: • a full bibliographic reference is made to the original source • a link is made to the metadata record in Durham E-Theses • the full-text is not changed in any way The full-text must not be sold in any format or medium without the formal permission of the copyright holders. Please consult the full Durham E-Theses policy for further details. Academic Support Oce, Durham University, University Oce, Old Elvet, Durham DH1 3HP e-mail: [email protected] Tel: +44 0191 334 6107 http://etheses.dur.ac.uk me91 In the name of Allah, the Gracious, the Merciful >° 9 43'' 0' eji e' e e> igo4 U61 J CO J: lic 6..ý v Lo ý , ý.,, "ý J ýs ýºý. ur ý,r11 Lýi is' ý9r ZU LZJE rju No disaster can befall on the earth or in your souls but it is in a book before We bring it into being; that is easy for Allah. In order that you may not grieve for what has escaped you, nor be exultant at what He has given you; and Allah does not love any prideful boaster.
    [Show full text]
  • 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.
    [Show full text]
  • Fy10 Budget by Program
    AURA/NOAO FISCAL YEAR ANNUAL REPORT FY 2010 Revised Submitted to the National Science Foundation March 16, 2011 This image, aimed toward the southern celestial pole atop the CTIO Blanco 4-m telescope, shows the Large and Small Magellanic Clouds, the Milky Way (Carinae Region) and the Coal Sack (dark area, close to the Southern Crux). The 33 “written” on the Schmidt Telescope dome using a green laser pointer during the two-minute exposure commemorates the rescue effort of 33 miners trapped for 69 days almost 700 m underground in the San Jose mine in northern Chile. The image was taken while the rescue was in progress on 13 October 2010, at 3:30 am Chilean Daylight Saving time. Image Credit: Arturo Gomez/CTIO/NOAO/AURA/NSF National Optical Astronomy Observatory Fiscal Year Annual Report for FY 2010 Revised (October 1, 2009 – September 30, 2010) Submitted to the National Science Foundation Pursuant to Cooperative Support Agreement No. AST-0950945 March 16, 2011 Table of Contents MISSION SYNOPSIS ............................................................................................................ IV 1 EXECUTIVE SUMMARY ................................................................................................ 1 2 NOAO ACCOMPLISHMENTS ....................................................................................... 2 2.1 Achievements ..................................................................................................... 2 2.2 Status of Vision and Goals ................................................................................
    [Show full text]
  • INAUGURAL – DISSERTATION Dipl.-Phys. Alexander A. Schegerer
    INAUGURAL – DISSERTATION zur Erlangung der Doktorwurde¨ der Naturwissenschaftlich-Mathematischen Gesamtfakult¨at der Ruprecht - Karls - Universit¨at Heidelberg vorgelegt von Dipl.-Phys. Alexander A. Schegerer, geboren in Kaufbeuren Tag der mundlichen¨ Prufung:¨ 17. Oktober 2007 II Struktur- und Staubentwicklung in zirkumstellaren Scheiben um T Tauri-Sterne Analyse und Modellierung hochaufl¨osender Beobachtungen in verschiedenen Wellenl¨angenbereichen Gutachter: Prof. Dr. Thomas Henning Prof. Dr. Wolfgang Duschl IV Meinen Eltern, Maria-Christa und Wolfgang Schegerer, gewidmet. VI Thema Im Zentrum dieser Doktorarbeit steht die Untersuchung der inneren Strukturen zirkumstella- rer Scheiben um T Tauri-Sterne sowie die Analyse zirkumstellarer Staub- und Eisteilchen und ihres Einflusses auf die Scheibenstruktur. Unter Zuhilfenahme von theoretisch berechneten Vergleichsspektren gibt der Verlauf der 10 µm-Emissionsbande in den Spektren junger stellarer Objekte Hinweise auf den Entwick- lungsgrad von Silikatstaub. Die Silikatbanden von 27 T Tauri-Objekten werden analysiert, um nach potentiell vorliegenden Korrelationen zwischen der Silikatstaubzusammensetzung und den stellaren Eigenschaften zu suchen. Analog erlaubt das Absorptionsband bei 3 µm, das dem Wassereis zugeschrieben wird, eine Untersuchung der Entwicklung von Eisk¨ornern in jungen stellaren Objekten. Erstmals ist es gelungen, kristallines Wassereis im Spektrum eines T Tauri-Objektes nachzuweisen. Unser wichtigstes Hilfsmittel zur Analyse der Temperatur- und Dichtestrukturen zirkum- stellarer
    [Show full text]
  • Instrumental Methods for Professional and Amateur
    Instrumental Methods for Professional and Amateur Collaborations in Planetary Astronomy Olivier Mousis, Ricardo Hueso, Jean-Philippe Beaulieu, Sylvain Bouley, Benoît Carry, Francois Colas, Alain Klotz, Christophe Pellier, Jean-Marc Petit, Philippe Rousselot, et al. To cite this version: Olivier Mousis, Ricardo Hueso, Jean-Philippe Beaulieu, Sylvain Bouley, Benoît Carry, et al.. Instru- mental Methods for Professional and Amateur Collaborations in Planetary Astronomy. Experimental Astronomy, Springer Link, 2014, 38 (1-2), pp.91-191. 10.1007/s10686-014-9379-0. hal-00833466 HAL Id: hal-00833466 https://hal.archives-ouvertes.fr/hal-00833466 Submitted on 3 Jun 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. Instrumental Methods for Professional and Amateur Collaborations in Planetary Astronomy O. Mousis, R. Hueso, J.-P. Beaulieu, S. Bouley, B. Carry, F. Colas, A. Klotz, C. Pellier, J.-M. Petit, P. Rousselot, M. Ali-Dib, W. Beisker, M. Birlan, C. Buil, A. Delsanti, E. Frappa, H. B. Hammel, A.-C. Levasseur-Regourd, G. S. Orton, A. Sanchez-Lavega,´ A. Santerne, P. Tanga, J. Vaubaillon, B. Zanda, D. Baratoux, T. Bohm,¨ V. Boudon, A. Bouquet, L. Buzzi, J.-L. Dauvergne, A.
    [Show full text]
  • Observing List
    day month year Epoch 2000 local clock time: 4.00 Observing List for 24 7 2019 RA DEC alt az Constellation object mag A mag B Separation description hr min deg min 60 75 Andromeda Gamma Andromedae (*266) 2.3 5.5 9.8 yellow & blue green double star 2 3.9 42 19 73 111 Andromeda Pi Andromedae 4.4 8.6 35.9 bright white & faint blue 0 36.9 33 43 72 71 Andromeda STF 79 (Struve) 6 7 7.8 bluish pair 1 0.1 44 42 58 80 Andromeda 59 Andromedae 6.5 7 16.6 neat pair, both greenish blue 2 10.9 39 2 89 34 Andromeda NGC 7662 (The Blue Snowball) planetary nebula, fairly bright & slightly elongated 23 25.9 42 32.1 75 84 Andromeda M31 (Andromeda Galaxy) large sprial arm galaxy like the Milky Way 0 42.7 41 16 75 85 Andromeda M32 satellite galaxy of Andromeda Galaxy 0 42.7 40 52 75 82 Andromeda M110 (NGC205) satellite galaxy of Andromeda Galaxy 0 40.4 41 41 60 84 Andromeda NGC752 large open cluster of 60 stars 1 57.8 37 41 57 73 Andromeda NGC891 edge on galaxy, needle-like in appearance 2 22.6 42 21 89 173 Andromeda NGC7640 elongated galaxy with mottled halo 23 22.1 40 51 82 10 Andromeda NGC7686 open cluster of 20 stars 23 30.2 49 8 47 200 Aquarius 55 Aquarii, Zeta 4.3 4.5 2.1 close, elegant pair of yellow stars 22 28.8 0 -1 35 181 Aquarius 94 Aquarii 5.3 7.3 12.7 pale rose & emerald 23 19.1 -13 28 30 173 Aquarius 107 Aquarii 5.7 6.7 6.6 yellow-white & bluish-white 23 46 -18 41 26 221 Aquarius M72 globular cluster 20 53.5 -12 32 27 220 Aquarius M73 Y-shaped asterism of 4 stars 20 59 -12 38 40 181 Aquarius NGC7606 Galaxy 23 19.1 -8 29 28 219 Aquarius NGC7009
    [Show full text]
  • Pulsating Components in Binary and Multiple Stellar Systems---A
    Research in Astron. & Astrophys. Vol.15 (2015) No.?, 000–000 (Last modified: — December 6, 2014; 10:26 ) Research in Astronomy and Astrophysics Pulsating Components in Binary and Multiple Stellar Systems — A Catalog of Oscillating Binaries ∗ A.-Y. Zhou National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China; [email protected] Abstract We present an up-to-date catalog of pulsating binaries, i.e. the binary and multiple stellar systems containing pulsating components, along with a statistics on them. Compared to the earlier compilation by Soydugan et al.(2006a) of 25 δ Scuti-type ‘oscillating Algol-type eclipsing binaries’ (oEA), the recent col- lection of 74 oEA by Liakos et al.(2012), and the collection of Cepheids in binaries by Szabados (2003a), the numbers and types of pulsating variables in binaries are now extended. The total numbers of pulsating binary/multiple stellar systems have increased to be 515 as of 2014 October 26, among which 262+ are oscillating eclipsing binaries and the oEA containing δ Scuti componentsare updated to be 96. The catalog is intended to be a collection of various pulsating binary stars across the Hertzsprung-Russell diagram. We reviewed the open questions, advances and prospects connecting pulsation/oscillation and binarity. The observational implication of binary systems with pulsating components, to stellar evolution theories is also addressed. In addition, we have searched the Simbad database for candidate pulsating binaries. As a result, 322 candidates were extracted. Furthermore, a brief statistics on Algol-type eclipsing binaries (EA) based on the existing catalogs is given. We got 5315 EA, of which there are 904 EA with spectral types A and F.
    [Show full text]
  • Vente De 2 Ans Montés Samedi 14 Mai Breeze Le 13 Mai
    11saint-cloud Vente de 2 ans montés Samedi 14 mai Breeze le 13 mai en association avec Index_Alpha_14_05 24/03/11 19:09 Page 71 Index alphabétique Alphabetical index NomsNOM des yearlings . .SUF . .Nos LOT NOM LOT ALKATARA . .0142 N(FAB'S MELODY 2009) . .0030 AMESBURY . .0148 N(FACTICE 2009) . .0031 FORCE MAJEUR . .0003 N(FAR DISTANCE 2009) . .0032 JOHN TUCKER . .0103 N(FIN 2009) . .0034 LIBERTY CAT . .0116 N(FLAMES 2009) . .0035 LUCAYAN . .0051 N(FOLLE LADY 2009) . .0036 MARCILHAC . .0074 N(FRANCAIS 2009) . .0037 MOST WANTED . .0123 N(GENDER DANCE 2009) . .0038 N(ABBEYLEIX LADY 2009) . .0139 N(GERMANCE 2009) . .0039 N(ABINGTON ANGEL 2009) . .0140 N(GILT LINKED 2009) . .0040 N(AIR BISCUIT 2009) . .0141 N(GREAT LADY SLEW 2009) . .0041 N(ALL EMBRACING 2009) . .0143 N(GRIN AND DARE IT 2009) . .0042 N(AMANDIAN 2009) . .0144 N(HARIYA 2009) . .0043 N(AMAZON BEAUTY 2009) . .0145 N(HOH MY DARLING 2009) . .0044 N(AMY G 2009) . .0146 N(INFINITY 2009) . .0045 N(ANSWER DO 2009) . .0147 N(INKLING 2009) . .0046 N(ARES VALLIS 2009) . .0149 N(JUST WOOD 2009) . .0048 N(AUCTION ROOM 2009) . .0150 N(KACSA 2009) . .0049 N(AVEZIA 2009) . .0151 N(KASSARIYA 2009) . .0050 N(BARCONEY 2009) . .0152 N(LALINA 2009) . .0052 N(BASHFUL 2009) . .0153 N(LANDELA 2009) . .0053 N(BAYOURIDA 2009) . .0154 N(LES ALIZES 2009) . .0054 N(BEE EATER 2009) . .0155 N(LIBRE 2009) . .0055 N(BELLA FIORELLA 2009) . .0156 N(LOUELLA 2009) . .0056 N(BERKELEY LODGE 2009) . .0157 N(LUANDA 2009) . .0057 N(BLACK PENNY 2009) . .0158 N(LUNA NEGRA 2009) .
    [Show full text]
  • Popular Names of Deep Sky (Galaxies,Nebulae and Clusters) Viciana’S List
    POPULAR NAMES OF DEEP SKY (GALAXIES,NEBULAE AND CLUSTERS) VICIANA’S LIST 2ª version August 2014 There isn’t any astronomical guide or star chart without a list of popular names of deep sky objects. Given the huge amount of celestial bodies labeled only with a number, the popular names given to them serve as a friendly anchor in a broad and complicated science such as Astronomy The origin of these names is varied. Some of them come from mythology (Pleiades); others from their discoverer; some describe their shape or singularities; (for instance, a rotten egg, because of its odor); and others belong to a constellation (Great Orion Nebula); etc. The real popular names of celestial bodies are those that for some special characteristic, have been inspired by the imagination of astronomers and amateurs. The most complete list is proposed by SEDS (Students for the Exploration and Development of Space). Other sources that have been used to produce this illustrated dictionary are AstroSurf, Wikipedia, Astronomy Picture of the Day, Skymap computer program, Cartes du ciel and a large bibliography of THE NAMES OF THE UNIVERSE. If you know other name of popular deep sky objects and you think it is important to include them in the popular names’ list, please send it to [email protected] with at least three references from different websites. If you have a good photo of some of the deep sky objects, please send it with standard technical specifications and an optional comment. It will be published in the names of the Universe blog. It could also be included in the ILLUSTRATED DICTIONARY OF POPULAR NAMES OF DEEP SKY.
    [Show full text]
  • High-Precision Time-Series Photometry for the Discovery and Characterization of Transiting Exoplanets
    University of Louisville ThinkIR: The University of Louisville's Institutional Repository Electronic Theses and Dissertations 5-2015 High-precision time-series photometry for the discovery and characterization of transiting exoplanets. Karen Alicia Collins 1962- University of Louisville Follow this and additional works at: https://ir.library.louisville.edu/etd Part of the Astrophysics and Astronomy Commons, and the Physics Commons Recommended Citation Collins, Karen Alicia 1962-, "High-precision time-series photometry for the discovery and characterization of transiting exoplanets." (2015). Electronic Theses and Dissertations. Paper 2104. https://doi.org/10.18297/etd/2104 This Doctoral Dissertation is brought to you for free and open access by ThinkIR: The University of Louisville's Institutional Repository. It has been accepted for inclusion in Electronic Theses and Dissertations by an authorized administrator of ThinkIR: The University of Louisville's Institutional Repository. This title appears here courtesy of the author, who has retained all other copyrights. For more information, please contact [email protected]. HIGH-PRECISION TIME-SERIES PHOTOMETRY FOR THE DISCOVERY AND CHARACTERIZATION OF TRANSITING EXOPLANETS By Karen A. Collins B.S., Georgia Institute of Technology, 1984 M.S., Georgia Institute of Technology, 1990 M.S., University of Louisville, 2008 A Dissertation Submitted to the Faculty of the College of Arts and Sciences of the University of Louisville in Partial Fulfillment of the Requirements for the Degree of Doctor of Philosophy in Physics Department of Physics and Astronomy University of Louisville Louisville, Kentucky May 2015 HIGH-PRECISION TIME-SERIES PHOTOMETRY FOR THE DISCOVERY AND CHARACTERIZATION OF TRANSITING EXOPLANETS By Karen A. Collins B.S., Georgia Institute of Technology, 1984 M.S., Georgia Institute of Technology, 1990 M.S., University of Louisville, 2008 A Dissertation Approved On April 17, 2015 by the following Dissertation Committee: Dissertation Director Dr.
    [Show full text]
  • Meteor.Mcse.Hu
    MCSE 2016/3 meteor.mcse.hu A Mars négy arca SZJA 1%! Az MCSE adószáma: 19009162-2-43 A Tharsis-régió három pajzsvulkánja és az Olympus Mons a Mars Express 2014. június 29-én készült felvételén (ESA / DLR / FU Berlin / Justin Cowart). TARTALOM Áttörés a fizikában......................... 3 GW150914: elõször hallottuk az Univerzum zenéjét....................... 4 A csillagászat ............................ 8 meteorA Magyar Csillagászati Egyesület lapja Journal of the Hungarian Astronomical Association Csillagászati hírek ........................ 10 H–1300 Budapest, Pf. 148., Hungary 1037 Budapest, Laborc u. 2/C. A távcsövek világa TELEFON/FAX: (1) 240-7708, +36-70-548-9124 Egy „klasszikus” naptávcsõ születése ........ 18 E-MAIL: [email protected], Honlap: meteor.mcse.hu HU ISSN 0133-249X Szabadszemes jelenségek Kiadó: Magyar Csillagászati Egyesület Gyöngyházfényû felhõk – történelmi észlelés! .. 22 FÔSZERKESZTÔ: Mizser Attila A hónap asztrofotója: hajnali együttállás ....... 27 SZERKESZTÔBIZOTTSÁG: Dr. Fûrész Gábor, Dr. Kiss László, Dr. Kereszturi Ákos, Dr. Kolláth Zoltán, Bolygók Mizser Attila, Dr. Sánta Gábor, Sárneczky Krisztián, Mars-oppozíció 2014 .................... 28 Dr. Szabados László és Dr. Szalai Tamás SZÍNES ELÕKÉSZÍTÉS: KÁRMÁN STÚDIÓ Nap FELELÔS KIADÓ: AZ MCSE ELNÖKE Téli változékony Napok .................38 A Meteor elôfizetési díja 2016-ra: (nem tagok számára) 7200 Ft Hold Egy szám ára: 600 Ft Januári Hold .........................42 Az egyesületi tagság formái (2016) • rendes tagsági díj (jogi személyek számára is) Meteorok
    [Show full text]
  • Observing List
    day month year Epoch 2000 local clock time: 22.00 Observing List for 18 5 2019 RA DEC alt az Constellation object mag A mag B Separation description hr min deg min 10 305 Auriga M37 January Salt and Pepper Cluster rich, open cluster of 150 stars, very fine 5 52.4 32 33 20 315 Auriga IC2149 planetary nebula, stellar to small disk, slightly elongated 5 56.5 46 6.3 15 319 Auriga Capella 0.1 alignment star 5 16.6 46 0 21 303 Auriga UU Aurigae Magnitude 5.1-7.0 carbon star (AL# 36) 6 36.5 38 27 15 307 Auriga 37 Theta Aurigae 2.6 7.1 3.6 white & bluish stars 5 59.7 37 13 74 45 Bootes 17, Kappa Bootis 4.6 6.6 13.4 bright white primary & bluish secondary 14 13.5 51 47 73 47 Bootes 21, Iota Bootis 4.9 7.5 38.5 wide yellow & blue pair 14 16.2 51 22 57 131 Bootes 29, Pi Bootis 4.9 5.8 5.6 fine bright white pair 14 40.7 16 25 64 115 Bootes 36, Epsilon Bootis (Izar) (*311) (HIP72105) 2.9 4.9 2.8 golden & greenish-blue 14 45 27 4 57 124 Bootes 37, Xi Bootis 4.7 7 6.6 beautiful yellow & reddish orange pair 14 51.4 19 6 62 86 Bootes 51, Mu Bootis 4.3 7 108.3 primary of yellow & close orange BC pair 15 24.5 37 23 62 96 Bootes Delta Bootis 3.5 8.7 105 wide yellow & blue pair 15 15.5 33 19 62 138 Bootes Arcturus -0.11 alignment star 14 15.6 19 10.4 56 162 Bootes NGC5248 galaxy with bright stellar nucleus and oval halo 13 37.5 8 53 72 56 Bootes NGC5676 elongated galaxy with slightly brighter center 14 32.8 49 28 72 59 Bootes NGC5689 galaxy, elongated streak with prominent oval core 14 35.5 48 45 16 330 Camelopardalis 1 Camelopardalis 5.7 6.8 10.3 white &
    [Show full text]