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Ix Ophiuchi: a High-Velocity Star Near a Molecular Cloud G
The Astronomical Journal, 130:815–824, 2005 August # 2005. The American Astronomical Society. All rights reserved. Printed in U.S.A. IX OPHIUCHI: A HIGH-VELOCITY STAR NEAR A MOLECULAR CLOUD G. H. Herbig Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI 96822 Received 2005 March 24; accepted 2005 April 26 ABSTRACT The molecular cloud Barnard 59 is probably an outlier of the Upper Sco/ Oph complex. B59 contains several T Tauri stars (TTSs), but outside its northwestern edge are three other H -emission objects whose nature has been unclear: IX, KK, and V359 Oph. This paper is a discussion of all three and of a nearby Be star (HD 154851), based largely on Keck HIRES spectrograms obtained in 2004. KK Oph is a close (1B6) double. The brighter component is an HAeBe star, and the fainter is a K-type TTS. The complex BVR variations of the unresolved pair require both components to be variable. V359 Oph is a conventional TTS. Thus, these pre-main-sequence stars continue to be recognizable as such well outside the boundary of their parent cloud. IX Oph is quite different. Its absorption spec- trum is about type G, with many peculiarities: all lines are narrow but abnormally weak, with structures that depend on ion and excitation level and that vary in detail from month to month. It could be a spectroscopic binary of small amplitude. H and H are the only prominent emission lines. They are broad, with variable central reversals. How- ever, the most unusual characteristic of IX Oph is the very high (heliocentric) radial velocity: about À310 km sÀ1, common to all spectrograms, and very different from the radial velocity of B59, about À7kmsÀ1. -
Binocular Certificate Handbook
Irish Federation of Astronomical Societies Binocular Certificate Handbook How to see 110 extraordinary celestial sights with an ordinary pair of binoculars © John Flannery, South Dublin Astronomical Society, August 2004 No ordinary binoculars! This photograph by the author is of the delightfully whimsical frontage of the Chiat/Day advertising agency building on Main Street, Venice, California. Binocular Certificate Handbook page 1 IFAS — www.irishastronomy.org Introduction HETHER NEW to the hobby or advanced am- Wateur astronomer you probably already own Binocular Certificate Handbook a pair of a binoculars, the ideal instrument to casu- ally explore the wonders of the Universe at any time. Name _____________________________ Address _____________________________ The handbook you hold in your hands is an intro- duction to the realm far beyond the Solar System — _____________________________ what amateur astronomers call the “deep sky”. This is the abode of galaxies, nebulae, and stars in many _____________________________ guises. It is here that we set sail from Earth and are Telephone _____________________________ transported across many light years of space to the wonderful and the exotic; dense glowing clouds of E-mail _____________________________ gas where new suns are being born, star-studded sec- tions of the Milky Way, and the ghostly light of far- Observing beginner/intermediate/advanced flung galaxies — all are within the grasp of an ordi- experience (please circle one of the above) nary pair of binoculars. Equipment __________________________________ True, the fixed magnification of (most) binocu- IFAS club __________________________________ lars will not allow you get the detail provided by telescopes but their wide field of view is perfect for NOTES: Details will be treated in strictest confidence. -
Uranometría Argentina Bicentenario
URANOMETRÍA ARGENTINA BICENTENARIO Reedición electrónica ampliada, ilustrada y actualizada de la URANOMETRÍA ARGENTINA Brillantez y posición de las estrellas fijas, hasta la séptima magnitud, comprendidas dentro de cien grados del polo austral. Resultados del Observatorio Nacional Argentino, Volumen I. Publicados por el observatorio 1879. Con Atlas (1877) 1 Observatorio Nacional Argentino Dirección: Benjamin Apthorp Gould Observadores: John M. Thome - William M. Davis - Miles Rock - Clarence L. Hathaway Walter G. Davis - Frank Hagar Bigelow Mapas del Atlas dibujados por: Albert K. Mansfield Tomado de Paolantonio S. y Minniti E. (2001) Uranometría Argentina 2001, Historia del Observatorio Nacional Argentino. SECyT-OA Universidad Nacional de Córdoba, Córdoba. Santiago Paolantonio 2010 La importancia de la Uranometría1 Argentina descansa en las sólidas bases científicas sobre la cual fue realizada. Esta obra, cuidada en los más pequeños detalles, se debe sin dudas a la genialidad del entonces director del Observatorio Nacional Argentino, Dr. Benjamin A. Gould. Pero nada de esto se habría hecho realidad sin la gran habilidad, el esfuerzo y la dedicación brindada por los cuatro primeros ayudantes del Observatorio, John M. Thome, William M. Davis, Miles Rock y Clarence L. Hathaway, así como de Walter G. Davis y Frank Hagar Bigelow que se integraron más tarde a la institución. Entre éstos, J. M. Thome, merece un lugar destacado por la esmerada revisión, control de las posiciones y determinaciones de brillos, tal como el mismo Director lo reconoce en el prólogo de la publicación. Por otro lado, Albert K. Mansfield tuvo un papel clave en la difícil confección de los mapas del Atlas. La Uranometría Argentina sobresale entre los trabajos realizados hasta ese momento, por múltiples razones: Por la profundidad en magnitud, ya que llega por vez primera en este tipo de empresa a la séptima. -
Probing the Galactic Halo with RR Lyrae Stars I: the Catalog
DRAFT VERSION FEBRUARY 5, 2020 Preprint typeset using LATEX style emulateapj v. 12/16/11 PROBING THE GALACTIC HALO WITH RR LYRAE STARS I: THE CATALOG G.-C. LIU1 , Y. HUANG2,9 , H.-W. ZHANG3,4 , M.-S. XIANG5 , J.-J., REN6, B.-Q. CHEN2, H.-B. YUAN 7 ,C.WANG3, Y. YANG 2 , Z.-J. TIAN 8 , F. WANG 3,4 , X.-W. LIU2,9 Draft version February 5, 2020 ABSTRACT We present a catalog of 5,290 RR Lyrae stars (RRLs) with metallicities estimated from spectra of the LAMOST Experiment for Galactic Understanding and Exploration (LEGUE) and the Sloan Extension for Galactic Un- derstanding and Exploration (SEGUE) surveys. Nearly 70 per cent of them (3,642 objects) also have systemic radial velocities measured. Given the pulsating nature of RRLs, metallicity estimates are based on spectra of individual exposures, by matching them with the synthetic templates. The systemic radial velocities are mea- sured by fitting the observed velocity as a function of phase assuming an empirical pulsating velocity template curve. Various tests show that our analyses yield metallicities with a typical precision of 0.20dex and systemic radial velocities with uncertainties ranging from 5 to 21km s−1 (depending on the number of radial velocity measurements available for a given star). Based on the well calibrated near-infrared PMW 1Z or PMKs Z, and MV -[Fe/H] relations, precise distances are derived for these RRLs. Finally, we include Gaia DR2 proper mo- tions in our catalog. The catalog should be very useful for various Galactic studies, especially of the Galactic halo. -
Geological Survey
DBPAETMENT OP THE INTEKIOB BULLETIN OK THE UNITED STATES GEOLOGICAL SURVEY No. 49 WASHINGTON GOVERNMENT PRINTING OFFICE 1889 UNITED STATES GEOLOGICAL SUBVEY J. W. POWELL, DIKECTOE LATITUDES AND LONGITUDES OF CERTAIN POINTS IN MISSOURI, KANSAS, AND NEW MEXICO EGBERT SIMPSO]N WOODWARD WASHINGTON- GOVERNMENT PRINTING OFFICE 1889 CONTENTS. Page. Letter of transmittal......................................................... 7 (1) Determination of astronomical positions in Missouri, Kansas, and New Mexico .......................................................... 9 Descriptions of stations ..................................................... 9 (2) Oswego, Elk Falls, and Fort Scott, Eans.; Springfield and Bolivar, Mo.; Albuquerque, N.Mex .................................. ..... 9 Instruments and instrumental constants..................................... 11 (3) Instruments used at Saint Louis and their constants ...... .......... 11 (4) Instruments used at Wie field stations and their constants ........... 11 (5) Principal details of determination of constants of field instruments .. 12 Latitudes .......... .......... .............................................. 20 (6) Methods of observation; selection of stars; table of results.......... 20 (7) Combination of results from different pairs of stars by weights; table of definitive reoults ................................................ 32 Longitudes ................................................................. 39 (8) Program for time determination .................................... 39 -
Toimetused Acta Et Comentationes
EESTI VABARIIGI TARTU ÜLIKOOLI TOIMETUSED ACTA ET COMENTATIONES UNIVERSITATIS DORPATENSIS A MATHEMATICA, PHYSICA, MEDICA III \ TARTU 1922 v / -V, EESTI VABARIIGI TARTU ÜLIKOOLI TOIMETUSED ACTA ET COMHENTATIONES UNIVERSITATIS DORPATENSIS A MATHBMATICA, PHYSICA, MBDICA ffl TARTU 1922 K. Mattiesen'i trükk, Tartus Sisukord. — Index. 1. J. Narbutt. Von den Kurven für die freie und die innere Energie bei Schmelz- und Umwandlungsvorgängen. 2. ApBH1HTl b ToMCOHi (Arwid Thomson). ÖHaneHie aMMOHifiHbixt cojieft aua HHTama BHcmHxfB KyjibTypHhixfc pacTemii. Referat: Der Wert der Ammonsalze für die Ernährung der höheren Kulturpflanzen. 3. Ernst Blessig. Ophthalmologische Bibliographie Russlands 1870—1920. I. Hälfte (S. I—VIl und 1—96). 4. A. Lüüs. Ein Beitrag zum Studium der Wirkung künstlicher Wil- dunger Hielenenquellensalze auf die Diurese nierenkranker Kinder. 5. E. Öpik. A Statistical method of counting shooting stars and its application to the Perseid shower of 1920. 6. P. N. Kogerman. The chemical composition of the Esthonian M.-Ordovician oil-bearing mineral „Kukersite". 7. M. Wittlich und S. Weshnjakow. Beitrag zur Kenntnis des est- ländischen Ölschiefers, genannt Kukkersit. Miseellanea: J. Letzmann. Die Trombe von Odenpäh am 10. Mai 1920. ,VON DEN KURVEN FÜR DIE FREIE UND DIE INNERE ENERGIE BEI SCHMELZ- UND UMWANDLUNGSVORGÄNGEN VON * J. NARBUTT DORPAT 1922 4 m * Druck von C. Mattiesen In einer früheren Arbeitx) habe ich in den Formeln für die freie Energie und für die Gesamtenergie bei Vorgängen in kon- densierten Einstoffsystemen an Stelle von T die reduzierte Um- wandlungs- resp. Schmelztemperatur #2) eingeführt und dadurch einige auf Umwandlungs- resp. Erstarrungsvorgänge u. s. w. bezügliche Schlüsse ziehen können. Weil die damalige Ableitung zuerst nicht auf die genannten Vorgänge beschränkt und des- halb allgemeiner geführt wurde, musste zur Auswertung der Integrationskonstante die Gültigkeit der anfangs gemachten spe- ziellen Annahme für die Temperaturabhängigkeit der Entropie bis zum absoluten Nullpunkt ausgedehnt werden. -