THE F@Qal Poilnt
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
October 2006
OCTOBER 2 0 0 6 �������������� http://www.universetoday.com �������������� TAMMY PLOTNER WITH JEFF BARBOUR 283 SUNDAY, OCTOBER 1 In 1897, the world’s largest refractor (40”) debuted at the University of Chica- go’s Yerkes Observatory. Also today in 1958, NASA was established by an act of Congress. More? In 1962, the 300-foot radio telescope of the National Ra- dio Astronomy Observatory (NRAO) went live at Green Bank, West Virginia. It held place as the world’s second largest radio scope until it collapsed in 1988. Tonight let’s visit with an old lunar favorite. Easily seen in binoculars, the hexagonal walled plain of Albategnius ap- pears near the terminator about one-third the way north of the south limb. Look north of Albategnius for even larger and more ancient Hipparchus giving an almost “figure 8” view in binoculars. Between Hipparchus and Albategnius to the east are mid-sized craters Halley and Hind. Note the curious ALBATEGNIUS AND HIPPARCHUS ON THE relationship between impact crater Klein on Albategnius’ southwestern wall and TERMINATOR CREDIT: ROGER WARNER that of crater Horrocks on the northeastern wall of Hipparchus. Now let’s power up and “crater hop”... Just northwest of Hipparchus’ wall are the beginnings of the Sinus Medii area. Look for the deep imprint of Seeliger - named for a Dutch astronomer. Due north of Hipparchus is Rhaeticus, and here’s where things really get interesting. If the terminator has progressed far enough, you might spot tiny Blagg and Bruce to its west, the rough location of the Surveyor 4 and Surveyor 6 landing area. -
And – Objektauswahl NGC Teil 1
And – Objektauswahl NGC Teil 1 NGC 5 NGC 49 NGC 79 NGC 97 NGC 184 NGC 233 NGC 389 NGC 531 Teil 1 NGC 11 NGC 51 NGC 80 NGC 108 NGC 205 NGC 243 NGC 393 NGC 536 NGC 13 NGC 67 NGC 81 NGC 109 NGC 206 NGC 252 NGC 404 NGC 542 Teil 2 NGC 19 NGC 68 NGC 83 NGC 112 NGC 214 NGC 258 NGC 425 NGC 551 NGC 20 NGC 69 NGC 85 NGC 140 NGC 218 NGC 260 NGC 431 NGC 561 NGC 27 NGC 70 NGC 86 NGC 149 NGC 221 NGC 262 NGC 477 NGC 562 NGC 29 NGC 71 NGC 90 NGC 160 NGC 224 NGC 272 NGC 512 NGC 573 NGC 39 NGC 72 NGC 93 NGC 169 NGC 226 NGC 280 NGC 523 NGC 590 NGC 43 NGC 74 NGC 94 NGC 181 NGC 228 NGC 304 NGC 528 NGC 591 NGC 48 NGC 76 NGC 96 NGC 183 NGC 229 NGC 317 NGC 529 NGC 605 Sternbild- Zur Objektauswahl: Nummer anklicken Übersicht Zur Übersichtskarte: Objekt in Aufsuchkarte anklicken Zum Detailfoto: Objekt in Übersichtskarte anklicken And – Objektauswahl NGC Teil 2 NGC 620 NGC 709 NGC 759 NGC 891 NGC 923 NGC 1000 NGC 7440 NGC 7836 Teil 1 NGC 662 NGC 710 NGC 797 NGC 898 NGC 933 NGC 7445 NGC 668 NGC 712 NGC 801 NGC 906 NGC 937 NGC 7446 Teil 2 NGC 679 NGC 714 NGC 812 NGC 909 NGC 946 NGC 7449 NGC 687 NGC 717 NGC 818 NGC 910 NGC 956 NGC 7618 NGC 700 NGC 721 NGC 828 NGC 911 NGC 980 NGC 7640 NGC 703 NGC 732 NGC 834 NGC 912 NGC 982 NGC 7662 NGC 704 NGC 746 NGC 841 NGC 913 NGC 995 NGC 7686 NGC 705 NGC 752 NGC 845 NGC 914 NGC 996 NGC 7707 NGC 708 NGC 753 NGC 846 NGC 920 NGC 999 NGC 7831 Sternbild- Zur Objektauswahl: Nummer anklicken Übersicht Zur Übersichtskarte: Objekt in Aufsuchkarte anklicken Zum Detailfoto: Objekt in Übersichtskarte anklicken Auswahl And SternbildübersichtAnd -
7.5 X 11.5.Threelines.P65
Cambridge University Press 978-0-521-19267-5 - Observing and Cataloguing Nebulae and Star Clusters: From Herschel to Dreyer’s New General Catalogue Wolfgang Steinicke Index More information Name index The dates of birth and death, if available, for all 545 people (astronomers, telescope makers etc.) listed here are given. The data are mainly taken from the standard work Biographischer Index der Astronomie (Dick, Brüggenthies 2005). Some information has been added by the author (this especially concerns living twentieth-century astronomers). Members of the families of Dreyer, Lord Rosse and other astronomers (as mentioned in the text) are not listed. For obituaries see the references; compare also the compilations presented by Newcomb–Engelmann (Kempf 1911), Mädler (1873), Bode (1813) and Rudolf Wolf (1890). Markings: bold = portrait; underline = short biography. Abbe, Cleveland (1838–1916), 222–23, As-Sufi, Abd-al-Rahman (903–986), 164, 183, 229, 256, 271, 295, 338–42, 466 15–16, 167, 441–42, 446, 449–50, 455, 344, 346, 348, 360, 364, 367, 369, 393, Abell, George Ogden (1927–1983), 47, 475, 516 395, 395, 396–404, 406, 410, 415, 248 Austin, Edward P. (1843–1906), 6, 82, 423–24, 436, 441, 446, 448, 450, 455, Abbott, Francis Preserved (1799–1883), 335, 337, 446, 450 458–59, 461–63, 470, 477, 481, 483, 517–19 Auwers, Georg Friedrich Julius Arthur v. 505–11, 513–14, 517, 520, 526, 533, Abney, William (1843–1920), 360 (1838–1915), 7, 10, 12, 14–15, 26–27, 540–42, 548–61 Adams, John Couch (1819–1892), 122, 47, 50–51, 61, 65, 68–69, 88, 92–93, -
High-Resolution Imaging of Transiting Extrasolar Planetary Systems (HITEP) II
A&A 610, A20 (2018) Astronomy DOI: 10.1051/0004-6361/201731855 & c ESO 2018 Astrophysics High-resolution Imaging of Transiting Extrasolar Planetary systems (HITEP) II. Lucky Imaging results from 2015 and 2016?,?? D. F. Evans1, J. Southworth1, B. Smalley1, U. G. Jørgensen2, M. Dominik3, M. I. Andersen4, V. Bozza5; 6, D. M. Bramich???, M. J. Burgdorf7, S. Ciceri8, G. D’Ago9, R. Figuera Jaimes3; 10, S.-H. Gu11; 12, T. C. Hinse13, Th. Henning8, M. Hundertmark14, N. Kains15, E. Kerins16, H. Korhonen4; 17, R. Kokotanekova18; 19, M. Kuffmeier2, P. Longa-Peña20, L. Mancini21; 8; 22, J. MacKenzie2, A. Popovas2, M. Rabus23; 8, S. Rahvar24, S. Sajadian25, C. Snodgrass19, J. Skottfelt19, J. Surdej26, R. Tronsgaard27, E. Unda-Sanzana20, C. von Essen27, Yi-Bo Wang11; 12, and O. Wertz28 (Affiliations can be found after the references) Received 29 August 2017 / Accepted 21 September 2017 ABSTRACT Context. The formation and dynamical history of hot Jupiters is currently debated, with wide stellar binaries having been suggested as a potential formation pathway. Additionally, contaminating light from both binary companions and unassociated stars can significantly bias the results of planet characterisation studies, but can be corrected for if the properties of the contaminating star are known. Aims. We search for binary companions to known transiting exoplanet host stars, in order to determine the multiplicity properties of hot Jupiter host stars. We also search for and characterise unassociated stars along the line of sight, allowing photometric and spectroscopic observations of the planetary system to be corrected for contaminating light. Methods. We analyse lucky imaging observations of 97 Southern hemisphere exoplanet host stars, using the Two Colour Instrument on the Danish 1.54 m telescope. -
Kinematics of the Local Universe
ASTRONOMY & ASTROPHYSICS JUNE I 1998, PAGE 333 SUPPLEMENT SERIES Astron. Astrophys. Suppl. Ser. 130, 333–339 (1998) Kinematics of the local universe VII. New 21-cm line measurements of 2112 galaxies?,?? G. Theureau1, L. Bottinelli1,3, N. Coudreau-Durand1, L. Gouguenheim1,3, N. Hallet1, M. Loulergue1, G. Paturel4, and P. Teerikorpi2 1 Observatoire de Paris/Meudon, ARPEGES/CNRS URA1757, F-92195 Meudon Principal Cedex, France 2 Tuorla Observatory, 21500 Piikki¨o, Finland 3 Universit´e Paris-Sud, F-91405 Orsay, France 4 Observatoire de Lyon, F-69561 Saint-Genis Laval Cedex, France Received November 28; accepted December 24, 1997 Abstract. This paper presents 2112 new 21-cm neutral hy- • the completeness of the sample (Paturel et al. 1994) drogen line measurements carried out with the meridian • the homogenization of optical and radio data in con- transit Nan¸cay radiotelescope. Among these data we give nexion with the Lyon-Meudon Extragalactic database also 213 new radial velocities which complement those LEDA (Bottinelli et al. 1990) listed in three previous papers of this series. These new • the effect of disc opaqueness on observed optical B- measurements, together with the HI data collected in band parameters (Bottinelli et al. 1995) LEDA, put to 6 700 the number of galaxies with 21-cm • the dependence of the TF relation on morphological line width, radial velocity, and apparent diameter in the type and mean surface brightness and the improve- so-called KLUN sample. ment of this distance indicator (Theureau et al. 1997a; Theureau 1998) Key words: catalogs — galaxies: distances and redshifts; • the determination of the Hubble constant H0 from TF ISM — radio lines: galaxies B-band and log D25 relations (Theureau et al. -
Making a Sky Atlas
Appendix A Making a Sky Atlas Although a number of very advanced sky atlases are now available in print, none is likely to be ideal for any given task. Published atlases will probably have too few or too many guide stars, too few or too many deep-sky objects plotted in them, wrong- size charts, etc. I found that with MegaStar I could design and make, specifically for my survey, a “just right” personalized atlas. My atlas consists of 108 charts, each about twenty square degrees in size, with guide stars down to magnitude 8.9. I used only the northernmost 78 charts, since I observed the sky only down to –35°. On the charts I plotted only the objects I wanted to observe. In addition I made enlargements of small, overcrowded areas (“quad charts”) as well as separate large-scale charts for the Virgo Galaxy Cluster, the latter with guide stars down to magnitude 11.4. I put the charts in plastic sheet protectors in a three-ring binder, taking them out and plac- ing them on my telescope mount’s clipboard as needed. To find an object I would use the 35 mm finder (except in the Virgo Cluster, where I used the 60 mm as the finder) to point the ensemble of telescopes at the indicated spot among the guide stars. If the object was not seen in the 35 mm, as it usually was not, I would then look in the larger telescopes. If the object was not immediately visible even in the primary telescope – a not uncommon occur- rence due to inexact initial pointing – I would then scan around for it. -
Ngc Catalogue Ngc Catalogue
NGC CATALOGUE NGC CATALOGUE 1 NGC CATALOGUE Object # Common Name Type Constellation Magnitude RA Dec NGC 1 - Galaxy Pegasus 12.9 00:07:16 27:42:32 NGC 2 - Galaxy Pegasus 14.2 00:07:17 27:40:43 NGC 3 - Galaxy Pisces 13.3 00:07:17 08:18:05 NGC 4 - Galaxy Pisces 15.8 00:07:24 08:22:26 NGC 5 - Galaxy Andromeda 13.3 00:07:49 35:21:46 NGC 6 NGC 20 Galaxy Andromeda 13.1 00:09:33 33:18:32 NGC 7 - Galaxy Sculptor 13.9 00:08:21 -29:54:59 NGC 8 - Double Star Pegasus - 00:08:45 23:50:19 NGC 9 - Galaxy Pegasus 13.5 00:08:54 23:49:04 NGC 10 - Galaxy Sculptor 12.5 00:08:34 -33:51:28 NGC 11 - Galaxy Andromeda 13.7 00:08:42 37:26:53 NGC 12 - Galaxy Pisces 13.1 00:08:45 04:36:44 NGC 13 - Galaxy Andromeda 13.2 00:08:48 33:25:59 NGC 14 - Galaxy Pegasus 12.1 00:08:46 15:48:57 NGC 15 - Galaxy Pegasus 13.8 00:09:02 21:37:30 NGC 16 - Galaxy Pegasus 12.0 00:09:04 27:43:48 NGC 17 NGC 34 Galaxy Cetus 14.4 00:11:07 -12:06:28 NGC 18 - Double Star Pegasus - 00:09:23 27:43:56 NGC 19 - Galaxy Andromeda 13.3 00:10:41 32:58:58 NGC 20 See NGC 6 Galaxy Andromeda 13.1 00:09:33 33:18:32 NGC 21 NGC 29 Galaxy Andromeda 12.7 00:10:47 33:21:07 NGC 22 - Galaxy Pegasus 13.6 00:09:48 27:49:58 NGC 23 - Galaxy Pegasus 12.0 00:09:53 25:55:26 NGC 24 - Galaxy Sculptor 11.6 00:09:56 -24:57:52 NGC 25 - Galaxy Phoenix 13.0 00:09:59 -57:01:13 NGC 26 - Galaxy Pegasus 12.9 00:10:26 25:49:56 NGC 27 - Galaxy Andromeda 13.5 00:10:33 28:59:49 NGC 28 - Galaxy Phoenix 13.8 00:10:25 -56:59:20 NGC 29 See NGC 21 Galaxy Andromeda 12.7 00:10:47 33:21:07 NGC 30 - Double Star Pegasus - 00:10:51 21:58:39 -
Curriculum Vitae Teaching
Curriculum Vitae Darren L. DePoy Current Position: Rachal/Mitchell/Heep Endowed Professorship in Physics, Texas A&M Univ. Postal Address: Department of Physics & Astronomy Texas A&M University TAMU 4242 College Station, Texas 77843 E-mail Address: [email protected] Voice: 979-862-2082 or 979-458-7923 Fax: 979-845-2590 Education: B.S. in Physics, Massachusetts Institute of Technology, 1982 Ph.D. in Astronomy, Univ. of Hawaii, 1987 Appointments: Physics Lab Instructor, Wellesley College, 1981-1982 Postdoctoral Fellow, Kitt Peak National Observatory, 1987-1988 Postdoctoral Fellow, Cerro Tololo Inter-American Observatory, 1988-1990 Assistant Professor of Astronomy, Ohio State Univ., 1990-1996 Associate Professor of Astronomy, Ohio State Univ., 1996-2002 Professor of Astronomy, Ohio State Univ., 2002-2008 Vice Chair for Instrumentation, Dept. of Astronomy, Ohio State Univ., 2002-2007 Rachal/Mitchell/Heep Professor of Physics, Texas A&M University, 2008-present Publications and Presentations: See following pages for list Total citations according to ADS as of June 2010: 4621 Recent Close Collaborators G. J. Hill (UT-Austin), B. Flaugher (FNAL), A. Gould (Ohio State) Thesis Students and Postdoctoral Scholars Advised B. Ali, C. J. Burke, J. L. Marshall, P. Martini, J. Pepper, K. Sills, A. Stephens Graduate and Postdoctoral Advisors E. E. Becklin (UCLA/SOFIA), I. Gatley (NJIT) Refereed Publications (as of June 2010) Masses and Orbital Constraints for the OGLE-2006-BLG-109Lb,c Jupiter/Saturn Analog Planetary System, Bennett, D. P., and 78 others including D. L. DePoy, The Astrophysical Journal, 2010, 713, 837 Variability and stability in blazar jets on time-scales of years: optical polarization monitoring of OJ 287 in 2005-2009, Villforth, C., and 47 others including D. -
Publications of Richard W. Pogge
Publications Richard William Pogge Updated: 2021 March 10 Doctoral Dissertation “The Circumnuclear Environment of Nearby, Non-Interacting Seyfert Galaxies”, University of California, Santa Cruz, June 1988. (Abstract published in PASP, 100, 1296, 1988. See also #7, 8, 10, 11, & 12 below.) Papers Published in Peer-RevieWed Journals 1. “X-Ray, Radio, and Infrared Observations of the Rapid Burster (MXB 1730-335) During 1979 and 1980”, LaWrence, A., et al. (52 authors), 1983, ApJ, 267, 301 2. “The Spectra of Narrow-Line Seyfert 1 Galaxies”, Osterbrock, Donald E., & Pogge, Richard W. 1985, ApJ, 297, 166 3. “The Extended Narrow Emission-Line Region of NGC 7469 Revisited”, DeRobertis, M.M. Pogge, R.W. 1986, AJ, 91, 1026 4. “Star Forming Regions in Gas-Rich Lenticulars. I. Ha Imaging of an Initial Sample of Galaxies”, Pogge, Richard W., & Eskridge, Paul B. 1987, AJ, 93, 291 5. “FY Aquilae and the Gamma-Ray Burst Event of 1979 March 31”, Hartmann, Dieter, & Pogge, Richard W. 1987, ApJ, 318, 363 6. “Optical Spectra of Narrow Emission Line Palomar-Green Galaxies”, Osterbrock, Donald E., & Pogge, Richard W. 1987, ApJ, 323, 108 7. “The circumnuclear environment of the nearby non-interacting Seyfert galaxies NGC 5273 and NGC 3516”, Pogge, R. W., 1988, LNP, 307, 46 8. “An Extended Ionizing Radiation Cone from the Nucleus of the Seyfert 2 Galaxy NGC 1068”, Pogge, Richard W. 1988, ApJ, 328, 519 9. “Extended Ionized Gas in the Seyfert 2 Galaxy NGC 4388”, Pogge, Richard W. 1988, ApJ, 332, 702 10. “OTS 1809+314 and the Gamma-Ray Burst GB 790325b”, Hartmann, Dieter, Pogge, Richard W., Hurley, Kevin, Vrba, Frederick J., & Jennings, Mark C. -
The Seyfert Galaxy Population
FIELD GALAXIES MARKARIAN GALAXIES OPTICALLY SELECTED^ QUASARS (LOCAL! KVKRT MF.rRS A/1 INI S-mf—8648 THE SEYFERT GALAXY POPULATION a radio survey; luminosity functions; related objects THE SEYFERT GALAXY POPULATION a radio survey; luminosity functions; related objects proefschrift ter verkrijging van de graad van Doctor in de Wiskunde en Natuurwetenschappen aan de Rijksuniversiteit te Leiden, op gezag van de Rector Magnificus Dr. AAH. Kassenaar, hoogleraar in de Faculteit der Geneeskunde, volgens besluit van het College van Dekanen te verdedigen op maandag 14 juni 1982 te klokke 14.15 uur door Evert Johan Alexander Meurs geboren te Amsterdam in 1950 Sterrewacht Leiden 1982 Beugelsdijk Leiden B.V. r Promotor: Prof. Dr. H. van der Laan Referenten: Prof. Dr. H.C. van de Hulst Dr. A.G. de Bruyn Voor mijn noeder, in herinnering, en voor Wouter TABLE OF CONTENTS CHAPTER I INTRODUCTION AND SYNOPSIS page 1. Seyfert galaxies 2. Contents of this thesis CHAPTER II OPTICAL POSITIONS OF SEYFERT GALAXIES 15 1. Introduction 2. Accurate Optical Positions of Seyfert Galaxies A.S.Wilson and E.J.A. Meurs, 1978, As iron.As trophys. Suppl.Ser. 33_,407 3. Further measurements CHAPTER III A RADIO SURVEY OF SEYFERT GALAXIES 25 1. A 1415 MHz Survey of Seyfert and Related Galaxies-II E.J.A. Meurs and A.S. Wilson, 1981, Astron.Astrophys. Suppl.Ser. 45,99 2. A 14)5 MHz Survey of Seyfert and Related Galaxies-III (In collaboration with A.S. Wilson.) CHAPTER IV LUMINOSITY FUNCTIONS OF SEYFERT GALAXIES 57 1. Introduction 2. Observational data 3. The optical luminosity function of Seyfert galaxies 4. -
Gear-Flex Coupling
RATHI TRANSPOWER PVT. LTD. PUNE - INDIA PRODUCT MANUAL GEAR-FLEX COUPLING TYPE – LFG/LHG R-PM-G-01/02-01/14 Page 1 INDEX CONTENTS PAGE • Standard Features 3 • At a Glance 3 • Gear-flex Family 4 • Std. Material of Construction 4 • Ratings for Standard couplings 5 • Weight & M.I. for standard couplings 6 • Customized Gear-flex Specials 7 • Half Flex Couplings with Floating Shafts 7 • Spacer Couplings 8 • Reversed Hub Combinations 8 • Lubricants 9 • Requirements of API-671 9 • Selection of Size of Coupling 10 • Typical Service Factors 11-13 • Std. Tolerances for Finish Bore & Keyway 14 • Applications 14 • Gear-flex couplings equivalent to Competitor’s couplings 15-18 R-PM-G-01/02-01/14 Page 2 GEAR-FLEX COUPLING STANDARD FEATURES OF GEAR-FLEX COUPLING ♦ Less backlash. ♦ High power to weight ratio. ♦ Compact assembly. ♦ Accommodates angular, parallel & axial misalignments. ♦ Generally used up to 120°C. Can be used for higher temperatures by using proper grade of oil or grease. ♦ Can be dynamically balanced to the required grade as per ISO-1940. AT A GLANCE SIZES Full Flexible Type LFG - 100 to 119 (20 sizes) Half Flexible Type LHG - 100 to 110 (11 sizes) RATING RANGE TYPE LFG - 5.9 kW to 17454 kW @ 100 rpm TYPE LHG- 5.9 kW to 963 kW @ 100 rpm TORQUE RANGE TYPE LFG - 559 Nm to 1666744 Nm TYPE LHG- 559 Nm to 91922 Nm BORE RANGE TYPE LFG - 13 mm. to 710 mm. TYPE LHG- 13 mm. to 260 mm. ANGULAR MISALIGNMENT - 1.5° per gear mesh Maximum COMPLIANCE WITH API-671 SPECIFICATIONS, IF REQD. -
A Classical Morphological Analysis of Galaxies in the Spitzer Survey Of
Accepted for publication in the Astrophysical Journal Supplement Series A Preprint typeset using LTEX style emulateapj v. 03/07/07 A CLASSICAL MORPHOLOGICAL ANALYSIS OF GALAXIES IN THE SPITZER SURVEY OF STELLAR STRUCTURE IN GALAXIES (S4G) Ronald J. Buta1, Kartik Sheth2, E. Athanassoula3, A. Bosma3, Johan H. Knapen4,5, Eija Laurikainen6,7, Heikki Salo6, Debra Elmegreen8, Luis C. Ho9,10,11, Dennis Zaritsky12, Helene Courtois13,14, Joannah L. Hinz12, Juan-Carlos Munoz-Mateos˜ 2,15, Taehyun Kim2,15,16, Michael W. Regan17, Dimitri A. Gadotti15, Armando Gil de Paz18, Jarkko Laine6, Kar´ın Menendez-Delmestre´ 19, Sebastien´ Comeron´ 6,7, Santiago Erroz Ferrer4,5, Mark Seibert20, Trisha Mizusawa2,21, Benne Holwerda22, Barry F. Madore20 Accepted for publication in the Astrophysical Journal Supplement Series ABSTRACT The Spitzer Survey of Stellar Structure in Galaxies (S4G) is the largest available database of deep, homogeneous middle-infrared (mid-IR) images of galaxies of all types. The survey, which includes 2352 nearby galaxies, reveals galaxy morphology only minimally affected by interstellar extinction. This paper presents an atlas and classifications of S4G galaxies in the Comprehensive de Vaucouleurs revised Hubble-Sandage (CVRHS) system. The CVRHS system follows the precepts of classical de Vaucouleurs (1959) morphology, modified to include recognition of other features such as inner, outer, and nuclear lenses, nuclear rings, bars, and disks, spheroidal galaxies, X patterns and box/peanut structures, OLR subclass outer rings and pseudorings, bar ansae and barlenses, parallel sequence late-types, thick disks, and embedded disks in 3D early-type systems. We show that our CVRHS classifications are internally consistent, and that nearly half of the S4G sample consists of extreme late-type systems (mostly bulgeless, pure disk galaxies) in the range Scd-Im.