Cet – Objektauswahl NGC Seite 1

Total Page:16

File Type:pdf, Size:1020Kb

Cet – Objektauswahl NGC Seite 1 Cet – Objektauswahl NGC Seite 1 NGC 34 NGC 65 NGC 118 NGC 154 NGC 172 NGC 196 NGC 227 NGC 255 NGC 277 NGC 35 NGC 66 NGC 120 NGC 155 NGC 173 NGC 197 NGC 230 NGC 259 NGC 279 NGC 45 NGC 73 NGC 124 NGC 157 NGC 175 NGC 201 NGC 232 NGC 263 NGC 283 Seite 2 NGC 47 NGC 77 NGC 132 NGC 161 NGC 177 NGC 207 NGC 235 NGC 268 NGC 284 NGC 50 NGC 102 NGC 135 NGC 163 NGC 178 NGC 209 NGC 237 NGC 270 NGC 285 Seite 3 NGC 54 NGC 142 NGC 107 NGC 165 NGC 179 NGC 210 NGC 239 NGC 271 NGC 286 Seite 4 NGC 59 NGC 113 NGC 143 NGC 166 NGC 187 NGC 216 NGC 244 NGC 273 NGC 291 NGC 61 NGC 114 NGC 144 NGC 167 NGC 191 NGC 217 NGC 245 NGC 274 NGC 293 Seite 5 NGC 62 NGC 116 NGC 145 NGC 168 NGC 192 NGC 219 NGC 246 NGC 275 NGC 297 NGC 64 NGC 117 NGC 151 NGC 170 NGC 195 NGC 223 NGC 247 NGC 276 NGC 298 Sternbild- Zur Objektauswahl: Nummer anklicken Übersicht Zur Übersichtskarte: Objekt in Aufsuchkarte anklicken Zum Detailfoto: Objekt in Übersichtskarte anklicken Cet – Objektauswahl NGC Seite 2 NGC 301 NGC 333 NGC 347 NGC 363 NGC 430 NGC 493 NGC 541 NGC 558 NGC 585 NGC 303 NGC 335 NGC 349 NGC 364 NGC 435 NGC 497 NGC 543 NGC 560 NGC 586 Seite 1 NGC 307 NGC 336 NGC 350 NGC 369 NGC 442 NGC 519 NGC 545 NGC 564 NGC 589 NGC 309 NGC 337 NGC 351 NGC 377 NGC 445 NGC 521 NGC 547 NGC 565 NGC 593 NGC 320 NGC 340 NGC 352 NGC 391 NGC 448 NGC 530 NGC 548 NGC 567 NGC 594 Seite 3 NGC 321 NGC 341 NGC 353 NGC 413 NGC 450 NGC 533 NGC 550 NGC 570 NGC 596 Seite 4 NGC 325 NGC 342 NGC 355 NGC 417 NGC 478 NGC 535 NGC 554 NGC 577 NGC 599 NGC 327 NGC 343 NGC 356 NGC 426 NGC 480 NGC 538 NGC 555 NGC 578 NGC 600 Seite 5 NGC 329 NGC 344 NGC 357 NGC 428 NGC 481 NGC 539 NGC 556 NGC 583 NGC 601 NGC 331 NGC 345 NGC 359 NGC 429 NGC 487 NGC 540 NGC 557 NGC 584 NGC 615 Sternbild- Zur Objektauswahl: Nummer anklicken Übersicht Zur Übersichtskarte: Objekt in Aufsuchkarte anklicken Zum Detailfoto: Objekt in Übersichtskarte anklicken Cet – Objektauswahl NGC Seite 3 NGC 617 NGC 667 NGC 720 NGC 758 NGC 800 NGC 831 NGC 848 NGC 872 NGC 892 NGC 622 NGC 681 NGC 723 NGC 762 NGC 806 NGC 833 NGC 849 NGC 873 NGC 894 Seite 1 NGC 624 NGC 682 NGC 725 NGC 767 NGC 808 NGC 835 NGC 850 NGC 874 NGC 895 Seite 2 NGC 635 NGC 690 NGC 726 NGC 768 NGC 809 NGC 836 NGC 851 NGC 875 NGC 899 NGC 636 NGC 699 NGC 731 NGC 773 NGC 811 NGC 837 NGC 853 NGC 878 NGC 902 NGC 640 NGC 701 NGC 734 NGC 779 NGC 814 NGC 838 NGC 856 NGC 879 NGC 905 Seite 4 NGC 647 NGC 702 NGC 747 NGC 787 NGC 815 NGC 839 NGC 858 NGC 880 NGC 907 NGC 648 NGC 707 NGC 748 NGC 788 NGC 825 NGC 840 NGC 863 NGC 881 NGC 908 Seite 5 NGC 649 NGC 713 NGC 755 NGC 790 NGC 827 NGC 842 NGC 864 NGC 883 NGC 921 NGC 655 NGC 715 NGC 756 NGC 799 NGC 829 NGC 844 NGC 868 NGC 887 NGC 926 NGC 830 Sternbild- Zur Objektauswahl: Nummer anklicken Übersicht Zur Übersichtskarte: Objekt in Aufsuchkarte anklicken Zum Detailfoto: Objekt in Übersichtskarte anklicken Cet – Objektauswahl NGC Seite 4 NGC 929 NGC 950 NGC 981 NGC 1008 NGC 1020 NGC 1042 NGC 1063 NGC 1075 Seite 1 NGC 934 NGC 955 NGC 985 NGC 1009 NGC 1021 NGC 1043 NGC 1064 NGC 1076 Seite 2 NGC 936 NGC 958 NGC 988 NGC 1010 NGC 1022 NGC 1044 NGC 1065 NGC 1078 NGC 941 NGC 960 NGC 989 NGC 1011 NGC 1026 NGC 1045 NGC 1068 NGC 1080 Seite 3 NGC 942 NGC 963 NGC 991 NGC 1013 NGC 1032 NGC 1046 NGC 1069 NGC 1085 NGC 943 NGC 965 NGC 993 NGC 1015 NGC 1033 NGC 1047 NGC 1070 NGC 1087 NGC 944 NGC 966 NGC 997 NGC 1016 NGC 1034 NGC 1048 NGC 1071 NGC 1090 NGC 945 NGC 967 NGC 998 NGC 1017 NGC 1035 NGC 1051 NGC 1072 Seite 5 NGC 947 NGC 975 NGC 1004 NGC 1018 NGC 1038 NGC 1052 NGC 1073 NGC 1094 NGC 948 NGC 977 NGC 1007 NGC 1019 NGC 1041 NGC 1055 NGC 1074 NGC 1095 Sternbild- Zur Objektauswahl: Nummer anklicken Übersicht Zur Übersichtskarte: Objekt in Aufsuchkarte anklicken Zum Detailfoto: Objekt in Übersichtskarte anklicken Cet – Objektauswahl NGC Seite 5 NGC 1101 NGC 1211 NGC 7807 Seite 1 NGC 1104 NGC 1218 NGC 7808 Seite 2 NGC 1107 NGC 1219 NGC 7813 NGC 1128 NGC 1254 NGC 7821 Seite 3 NGC 1137 NGC 1280 NGC 7828 NGC 1143 NGC 7829 Seite 4 NGC 1144 NGC 1149 NGC 1153 NGC 1194 Sternbild- Zur Objektauswahl: Nummer anklicken Übersicht Zur Übersichtskarte: Objekt in Aufsuchkarte anklicken Zum Detailfoto: Objekt in Übersichtskarte anklicken Cet Übersichtskarte Auswahl NGC 34_35_7808_7813_7828_7829 Aufsuchkarte Auswahl NGC 45_59_65_66_77 Aufsuchkarte Auswahl NGC 47_50_54_61_64 Aufsuchkarte Auswahl NGC 62_73_102 Aufsuchkarte Auswahl NGC 107_116_145 Aufsuchkarte Auswahl NGC 113_114_118_120_124_161 Aufsuchkarte Auswahl NGC 117_132 Aufsuchkarte Auswahl NGC 135_154_166_178_179_187_207_210 Aufsuchkarte Auswahl NGC 142_143_144_167_168_172_177_216_230_232_235 Aufsuchkarte Auswahl NGC 151_155_157_163_165_191_195_217 Aufsuchkarte Auswahl NGC 170_173_192_196_197_201_219_223_237 Aufsuchkarte Auswahl NGC 175_209 Aufsuchkarte Auswahl NGC 227_239_245_259_271_279 Aufsuchkarte 20 Cet20 Auswahl NGC 244_303_333_363_369 Aufsuchkarte Auswahl NGC 246_255_263_283_284_285_286 Aufsuchkarte Auswahl NGC 247_276_320_335_336_343_344_377_417 Aufsuchkarte 166528 SAO Auswahl NGC 268_70_73_74_75_77_91_93_97_98_309_21_25_27_29_37_40 _41_42_45_47_49_50_52_55_56_57Aufsuchkarte Auswahl NGC 301 Aufsuchkarte Auswahl NGC 307_331_351_353_359_364 Aufsuchkarte Auswahl NGC 367 Aufsuchkarte Auswahl NGC 391_426_28_29_30_35_42_45_48_50 Aufsuchkarte Auswahl NGC 413 Aufsuchkarte Auswahl NGC 478_554_555_556_578 Aufsuchkarte Auswahl NGC 480_481_567_589_593_599_601_617_624_640_647_649 Aufsuchkarte Auswahl NGC 487_539_540_583_594_648 Aufsuchkarte Auswahl NGC 493_497_519_21_30_33_35_38_41_43_45_47_48_50_57_58_6 0_64_65_70_77_85_622 Aufsuchkarte Auswahl NGC 584_586_596_600_615_636 Aufsuchkarte Auswahl NGC 635_667_723 Aufsuchkarte Auswahl NGC 655 Aufsuchkarte Auswahl NGC 681 Aufsuchkarte Auswahl NGC 682_699_715_720_814_815 Aufsuchkarte Auswahl NGC 690_725_734_756 Aufsuchkarte Auswahl NGC 701_707 Aufsuchkarte Auswahl NGC 702_748_758_762_779_788_790 Aufsuchkarte Auswahl NGC 713_26_31_47_55_67_73_87_806_09_11_29_30_33_35_38_39_42_48_53_73_ 79 Aufsuchkarte Auswahl NGC 768_799_800_850_856_863_868_875 Aufsuchkarte Auswahl N 808_36_37_49_58_74_78_92_99_907_08_51 Aufsuchkarte Auswahl NGC 825_27_31_40_44_51_64 Aufsuchkarte Auswahl NGC 872_887_902_21_47_65_66_67_89 Aufsuchkarte Auswahl NGC 880_881_883_894_895 Aufsuchkarte Auswahl NGC 905 Aufsuchkarte Auswahl NGC 926_34_36_41_55_58_63_1015 Aufsuchkarte Auswahl N 929_42_43_45_48_50_60_77_81_85_88Aufsuchkarte Auswahl NGC 944 Aufsuchkarte Auswahl NGC 975_997_998_1026_1044_1046 Aufsuchkarte Auswahl NGC 991_1022_1041_1051_1063_1080 Aufsuchkarte 80 Cet 77 Cet Auswahl NGC 993_1004_07_08_09_16_19_20_21 Aufsuchkarte Auswahl NGC 1010_11_13_17_18_33_35_42_45_47_48_52_64_69_71_78 Aufsuchkarte Auswahl NGC 1032_1038_1043_1073 Aufsuchkarte Auswahl NGC 1034_1065_1074_1075_1076 Aufsuchkarte Auswahl NGC 1055_68_72_87_90_94_1104_43_44_49 Aufsuchkarte Auswahl NGC 1070_1085_1095_1101 Aufsuchkarte Auswahl NGC 1107 Aufsuchkarte Auswahl NGC 1128 Aufsuchkarte Auswahl NGC 1137_1153 Aufsuchkarte Auswahl NGC 1194_1211_1218_1219_1254_1280 Aufsuchkarte Auswahl NGC 7807_7821 Aufsuchkarte Auswahl NGC 34_35 Übersichtskarte Aufsuch- Auswahl karte NGC 45 Übersichtskarte Aufsuch- Auswahl karte NGC 47_50_54 Übersichtskarte Aufsuch- Auswahl karte NGC 59 Übersichtskarte Aufsuch- Auswahl karte NGC 61_64 Übersichtskarte Aufsuch- Auswahl karte NGC 62 Übersichtskarte Aufsuch- Auswahl karte NGC 65_66_77 Übersichtskarte Aufsuch- Auswahl karte NGC 73 Übersichtskarte Aufsuch- Auswahl karte NGC 102 Übersichtskarte Aufsuch- Auswahl karte NGC 107_116 Übersichtskarte Aufsuch- Auswahl karte NGC 113 Übersichtskarte Aufsuch- Auswahl karte NGC 114_118_120_124 Übersichtskarte Aufsuch- Auswahl karte NGC 117 Übersichtskarte Aufsuch- Auswahl karte NGC 132 Übersichtskarte Aufsuch- Auswahl karte NGC 135_154 Übersichtskarte Aufsuch- Auswahl karte NGC 142_143_144 Übersichtskarte Aufsuch- Auswahl karte NGC 145 Übersichtskarte Aufsuch- Auswahl karte NGC 151 Übersichtskarte Aufsuch- Auswahl karte NGC 155_163_165 Übersichtskarte Aufsuch- Auswahl karte NGC 157 Übersichtskarte Aufsuch- Auswahl karte NGC 161 Übersichtskarte Aufsuch- Auswahl karte NGC 166 Übersichtskarte Aufsuch- Auswahl karte NGC 167 Übersichtskarte Aufsuch- Auswahl karte NGC 168_172_177 Übersichtskarte Aufsuch- Auswahl karte NGC 170_173 Übersichtskarte Aufsuch- Auswahl karte NGC 175 Übersichtskarte Aufsuch- Auswahl karte NGC 178_187_207_210 Übersichtskarte Aufsuch- Auswahl karte NGC 179 Übersichtskarte Aufsuch- Auswahl karte NGC 191_195 Übersichtskarte Aufsuch- Auswahl karte NGC 192_196_197_201_219_223 Übersichtskarte Aufsuch- Auswahl karte NGC 209 Übersichtskarte Aufsuch- Auswahl karte NGC 216 Übersichtskarte Aufsuch- Auswahl karte NGC 217 Übersichtskarte Aufsuch- Auswahl karte NGC 227 Übersichtskarte Aufsuch- Auswahl karte NGC 230_232_235 Übersichtskarte Aufsuch- Auswahl karte NGC 237 Übersichtskarte Aufsuch- Auswahl karte NGC 239 Übersichtskarte Aufsuch- Auswahl karte NGC 244 Übersichtskarte Aufsuch- Auswahl karte NGC 245 Übersichtskarte Aufsuch- Auswahl karte NGC 246_255 Übersichtskarte Aufsuch- Auswahl karte NGC 247 Übersichtskarte Aufsuch- Auswahl karte NGC 259 Übersichtskarte Aufsuch- Auswahl karte NGC 263 Übersichtskarte Aufsuch- Auswahl karte NGC 268 Übersichtskarte Aufsuch- Auswahl karte NGC 270_277_291 Übersichtskarte Aufsuch- Auswahl karte NGC 271_279 Übersichtskarte Aufsuch- Auswahl karte NGC 273_274_275 Übersichtskarte Aufsuch- Auswahl karte NGC 276 Übersichtskarte Aufsuch- Auswahl karte NGC 283_284_285_286 Übersichtskarte Aufsuch- Auswahl karte NGC 293_297_298 Übersichtskarte Aufsuch- Auswahl karte NGC 301 Übersichtskarte Aufsuch- Auswahl karte NGC 303 Übersichtskarte Aufsuch-
Recommended publications
  • Infrared Spectroscopy of Nearby Radio Active Elliptical Galaxies
    The Astrophysical Journal Supplement Series, 203:14 (11pp), 2012 November doi:10.1088/0067-0049/203/1/14 C 2012. The American Astronomical Society. All rights reserved. Printed in the U.S.A. INFRARED SPECTROSCOPY OF NEARBY RADIO ACTIVE ELLIPTICAL GALAXIES Jeremy Mould1,2,9, Tristan Reynolds3, Tony Readhead4, David Floyd5, Buell Jannuzi6, Garret Cotter7, Laura Ferrarese8, Keith Matthews4, David Atlee6, and Michael Brown5 1 Centre for Astrophysics and Supercomputing Swinburne University, Hawthorn, Vic 3122, Australia; [email protected] 2 ARC Centre of Excellence for All-sky Astrophysics (CAASTRO) 3 School of Physics, University of Melbourne, Melbourne, Vic 3100, Australia 4 Palomar Observatory, California Institute of Technology 249-17, Pasadena, CA 91125 5 School of Physics, Monash University, Clayton, Vic 3800, Australia 6 Steward Observatory, University of Arizona (formerly at NOAO), Tucson, AZ 85719 7 Department of Physics, University of Oxford, Denys, Oxford, Keble Road, OX13RH, UK 8 Herzberg Institute of Astrophysics Herzberg, Saanich Road, Victoria V8X4M6, Canada Received 2012 June 6; accepted 2012 September 26; published 2012 November 1 ABSTRACT In preparation for a study of their circumnuclear gas we have surveyed 60% of a complete sample of elliptical galaxies within 75 Mpc that are radio sources. Some 20% of our nuclear spectra have infrared emission lines, mostly Paschen lines, Brackett γ , and [Fe ii]. We consider the influence of radio power and black hole mass in relation to the spectra. Access to the spectra is provided here as a community resource. Key words: galaxies: elliptical and lenticular, cD – galaxies: nuclei – infrared: general – radio continuum: galaxies ∼ 1. INTRODUCTION 30% of the most massive galaxies are radio continuum sources (e.g., Fabbiano et al.
    [Show full text]
  • CO Multi-Line Imaging of Nearby Galaxies (COMING) IV. Overview Of
    Publ. Astron. Soc. Japan (2018) 00(0), 1–33 1 doi: 10.1093/pasj/xxx000 CO Multi-line Imaging of Nearby Galaxies (COMING) IV. Overview of the Project Kazuo SORAI1, 2, 3, 4, 5, Nario KUNO4, 5, Kazuyuki MURAOKA6, Yusuke MIYAMOTO7, 8, Hiroyuki KANEKO7, Hiroyuki NAKANISHI9 , Naomasa NAKAI4, 5, 10, Kazuki YANAGITANI6 , Takahiro TANAKA4, Yuya SATO4, Dragan SALAK10, Michiko UMEI2 , Kana MOROKUMA-MATSUI7, 8, 11, 12, Naoko MATSUMOTO13, 14, Saeko UENO9, Hsi-An PAN15, Yuto NOMA10, Tsutomu, T. TAKEUCHI16 , Moe YODA16, Mayu KURODA6, Atsushi YASUDA4 , Yoshiyuki YAJIMA2 , Nagisa OI17, Shugo SHIBATA2, Masumichi SETA10, Yoshimasa WATANABE4, 5, 18, Shoichiro KITA4, Ryusei KOMATSUZAKI4 , Ayumi KAJIKAWA2, 3, Yu YASHIMA2, 3, Suchetha COORAY16 , Hiroyuki BAJI6 , Yoko SEGAWA2 , Takami TASHIRO2 , Miho TAKEDA6, Nozomi KISHIDA2 , Takuya HATAKEYAMA4 , Yuto TOMIYASU4 and Chey SAITA9 1Department of Physics, Faculty of Science, Hokkaido University, Kita 10 Nishi 8, Kita-ku, Sapporo 060-0810, Japan 2Department of Cosmosciences, Graduate School of Science, Hokkaido University, Kita 10 Nishi 8, Kita-ku, Sapporo 060-0810, Japan 3Department of Physics, School of Science, Hokkaido University, Kita 10 Nishi 8, Kita-ku, Sapporo 060-0810, Japan 4Division of Physics, Faculty of Pure and Applied Sciences, University of Tsukuba, 1-1-1 Tennodai, Tsukuba, Ibaraki 305-8571, Japan 5Tomonaga Center for the History of the Universe (TCHoU), University of Tsukuba, 1-1-1 Tennodai, Tsukuba, Ibaraki 305-8571, Japan 6Department of Physical Science, Osaka Prefecture University, Gakuen 1-1,
    [Show full text]
  • Circumstellar Material in Type Ia Supernovae Via Sodium Absorption
    Circumstellar Material in Type Ia Supernovae via Sodium Absorption Features A. Sternberg1∗, A. Gal-Yam1∗, J. D. Simon2, D. C. Leonard3, R. M. Quimby4, M. M. Phillips5, N. Morrell5, I. B. Thompson2, I. Ivans6, J. L. Marshall7, A. V. Filippenko8, G. W. Marcy8, J. S. Bloom8, F. Patat9, R. J. Foley10, D. Yong11, B. E. Penprase12, D. J. Beeler12, C. Allende Prieto13,14, G. S. Stringfellow15 1Benoziyo Center for Astrophysics, Faculty of Physics, Weizmann Institute of Science, Rehovot 76100, Israel. 2Observatories of the Carnegie Institution of Washington, 813 Santa Barbara St., Pasadena, CA 91101, USA. 3Department of Astronomy, San Diego State University, San Diego, CA 92182, USA. 4Cahill Center for Astrophysics, California Institute of Technology, Pasadena, CA 91125, USA. 5Carnegie Observatories, Las Campanas Observatory, Casilla 601, La Serena, Chile. 6Deparment of Physics & Astronomy, The University of Utah, Salt Lake City, UT 84112, USA. 7Department of Physics, Texas A&M University, 4242 TAMU, College Station, TX 77843, USA. 8Department of Astronomy, University of California, Berkeley, CA 94720-3411, USA. 9European Southern Observatory (ESO), Karl Schwarzschild Strasse 2, 85748, Garching bei M¨unchen, Germany. 10Clay Fellow, Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA. 11Research School of Astronomy & Astrophysics, The Australian National University, Mount Stromlo Observatory, Cotter Rd., Weston ACT 2611, Australia. 12Department of Physics and Astronomy, Pomona College, 610 N. College Ave., Claremont, CA 91711, USA. 13Instituto de Astrof´ısica de Canarias, 38205, La Laguna, Tenerife, Spain. arXiv:1108.3664v1 [astro-ph.HE] 18 Aug 2011 14Departamento de Astrof´ısica, Universidad de La Laguna, 38206, La Laguna, Tenerife, Spain.
    [Show full text]
  • Structure and Star Formation in Disk Galaxies I. Sample Selection And
    Mon. Not. R. Astron. Soc. 000, 1–9 (2003) Printed 31 October 2018 (MN LATEX style file v1.4) Structure and star formation in disk galaxies I. Sample selection and near infrared imaging J. H. Knapen1,2, R. S. de Jong3, S. Stedman1 and D. M. Bramich4 1University of Hertfordshire, Department of Physical Sciences, Hatfield, Herts AL10 9AB 2Isaac Newton Group of Telescopes, Apartado 321, E-38700 Santa Cruz de La Palma, Spain 3Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA 4School of Physics and Astronomy, University of St. Andrews, Scotland KY16 9SS Accepted March 2003. Received ; in original form ABSTRACT We present near-infrared imaging of a sample of 57 relatively large, Northern spiral galaxies with low inclination. After describing the selection criteria and some of the basic properties of the sample, we give a detailed description of the data collection and reduction procedures. The Ks λ =2.2µm images cover most of the disk for all galaxies, with a field of view of at least 4.2 arcmin. The spatial resolution is better than an arcsec for most images. We fit bulge and exponential disk components to radial profiles of the light distribution. We then derive the basic parameters of these components, as well as the bulge/disk ratio, and explore correlations of these parameters with several galaxy parameters. Key words: galaxies: spiral – galaxies: structure – infrared: galaxies 1 INTRODUCTION only now starting to be published (e.g., 2MASS: Skrutskie et al. 1997, Jarrett et al. 2003; Seigar & James 1998a, 1998b; Near-infrared (NIR) imaging of galaxies is a better tracer Moriondo et al.
    [Show full text]
  • Comprehensive Broadband X-Ray and Multiwavelength Study of Active Galactic Nuclei in Local 57 Ultra/Luminous Infrared Galaxies Observed with Nustar And/Or Swift/BAT
    Draft version July 26, 2021 Typeset using LATEX twocolumn style in AASTeX631 Comprehensive Broadband X-ray and Multiwavelength Study of Active Galactic Nuclei in Local 57 Ultra/luminous Infrared Galaxies Observed with NuSTAR and/or Swift/BAT Satoshi Yamada ,1 Yoshihiro Ueda ,1 Atsushi Tanimoto ,2 Masatoshi Imanishi ,3, 4 Yoshiki Toba ,1, 5 Claudio Ricci ,6, 7, 8 and George C. Privon 9 1Department of Astronomy, Kyoto University, Kitashirakawa-Oiwake-cho, Sakyo-ku, Kyoto 606-8502, Japan 2Department of Physics, The University of Tokyo, Tokyo 113-0033, Japan 3National Astronomical Observatory of Japan, Osawa, Mitaka, Tokyo 181-8588, Japan 4Department of Astronomical Science, Graduate University for Advanced Studies (SOKENDAI), 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan 5Research Center for Space and Cosmic Evolution, Ehime University, 2-5 Bunkyo-cho, Matsuyama, Ehime 790-8577, Japan 6N´ucleo de Astronom´ıade la Facultad de Ingenier´ıa,Universidad Diego Portales, Av. Ej´ercito Libertador 441, Santiago, Chile 7Kavli Institute for Astronomy and Astrophysics, Peking University, Beijing 100871, People's Republic of China 8George Mason University, Department of Physics & Astronomy, MS 3F3, 4400 University Drive, Fairfax, VA 22030, USA 9National Radio Astronomy Observatory, 520 Edgemont Rd, Charlottesville, VA 22903, USA (Received April 13, 2021; Revised June 11, 2021; Accepted Jul, 2021) ABSTRACT We perform a systematic X-ray spectroscopic analysis of 57 local ultra/luminous infrared galaxy systems (containing 84 individual galaxies) observed with Nuclear Spectroscopic Telescope Array and/or Swift/BAT. Combining soft X-ray data obtained with Chandra, XMM-Newton, Suzaku and/or Swift/XRT, we identify 40 hard (>10 keV) X-ray detected active galactic nuclei (AGNs) and con- strain their torus parameters with the X-ray clumpy torus model XCLUMPY (Tanimoto et al.
    [Show full text]
  • And Ecclesiastical Cosmology
    GSJ: VOLUME 6, ISSUE 3, MARCH 2018 101 GSJ: Volume 6, Issue 3, March 2018, Online: ISSN 2320-9186 www.globalscientificjournal.com DEMOLITION HUBBLE'S LAW, BIG BANG THE BASIS OF "MODERN" AND ECCLESIASTICAL COSMOLOGY Author: Weitter Duckss (Slavko Sedic) Zadar Croatia Pусскй Croatian „If two objects are represented by ball bearings and space-time by the stretching of a rubber sheet, the Doppler effect is caused by the rolling of ball bearings over the rubber sheet in order to achieve a particular motion. A cosmological red shift occurs when ball bearings get stuck on the sheet, which is stretched.“ Wikipedia OK, let's check that on our local group of galaxies (the table from my article „Where did the blue spectral shift inside the universe come from?“) galaxies, local groups Redshift km/s Blueshift km/s Sextans B (4.44 ± 0.23 Mly) 300 ± 0 Sextans A 324 ± 2 NGC 3109 403 ± 1 Tucana Dwarf 130 ± ? Leo I 285 ± 2 NGC 6822 -57 ± 2 Andromeda Galaxy -301 ± 1 Leo II (about 690,000 ly) 79 ± 1 Phoenix Dwarf 60 ± 30 SagDIG -79 ± 1 Aquarius Dwarf -141 ± 2 Wolf–Lundmark–Melotte -122 ± 2 Pisces Dwarf -287 ± 0 Antlia Dwarf 362 ± 0 Leo A 0.000067 (z) Pegasus Dwarf Spheroidal -354 ± 3 IC 10 -348 ± 1 NGC 185 -202 ± 3 Canes Venatici I ~ 31 GSJ© 2018 www.globalscientificjournal.com GSJ: VOLUME 6, ISSUE 3, MARCH 2018 102 Andromeda III -351 ± 9 Andromeda II -188 ± 3 Triangulum Galaxy -179 ± 3 Messier 110 -241 ± 3 NGC 147 (2.53 ± 0.11 Mly) -193 ± 3 Small Magellanic Cloud 0.000527 Large Magellanic Cloud - - M32 -200 ± 6 NGC 205 -241 ± 3 IC 1613 -234 ± 1 Carina Dwarf 230 ± 60 Sextans Dwarf 224 ± 2 Ursa Minor Dwarf (200 ± 30 kly) -247 ± 1 Draco Dwarf -292 ± 21 Cassiopeia Dwarf -307 ± 2 Ursa Major II Dwarf - 116 Leo IV 130 Leo V ( 585 kly) 173 Leo T -60 Bootes II -120 Pegasus Dwarf -183 ± 0 Sculptor Dwarf 110 ± 1 Etc.
    [Show full text]
  • 1987Apj. . .320. .2383 the Astrophysical Journal, 320:238-257
    .2383 The Astrophysical Journal, 320:238-257,1987 September 1 © 1987. The American Astronomical Society. AU rights reserved. Printed in U.S.A. .320. 1987ApJ. THE IRÁS BRIGHT GALAXY SAMPLE. II. THE SAMPLE AND LUMINOSITY FUNCTION B. T. Soifer, 1 D. B. Sanders,1 B. F. Madore,1,2,3 G. Neugebauer,1 G. E. Danielson,4 J. H. Elias,1 Carol J. Lonsdale,5 and W. L. Rice5 Received 1986 December 1 ; accepted 1987 February 13 ABSTRACT A complete sample of 324 extragalactic objects with 60 /mi flux densities greater than 5.4 Jy has been select- ed from the IRAS catalogs. Only one of these objects can be classified morphologically as a Seyfert nucleus; the others are all galaxies. The median distance of the galaxies in the sample is ~ 30 Mpc, and the median 10 luminosity vLv(60 /mi) is ~2 x 10 L0. This infrared selected sample is much more “infrared active” than optically selected galaxy samples. 8 12 The range in far-infrared luminosities of the galaxies in the sample is 10 LQ-2 x 10 L©. The far-infrared luminosities of the sample galaxies appear to be independent of the optical luminosities, suggesting a separate luminosity component. As previously found, a correlation exists between 60 /¿m/100 /¿m flux density ratio and far-infrared luminosity. The mass of interstellar dust required to produce the far-infrared radiation corre- 8 10 sponds to a mass of gas of 10 -10 M0 for normal gas to dust ratios. This is comparable to the mass of the interstellar medium in most galaxies.
    [Show full text]
  • 194 9 Ce Le B Rating 65 Ye Ars O F Br Inging As Tr on Omy T O No Rth Te X As 2
    1949 Celebrating 65 Years of Bringing Astronomy to North Texas 2014 Contact information: Inside this issue: Info Officer (General Info) – [email protected] Website Administrator – [email protected] Page Postal Address: November Club Calendar 3 Fort Worth Astronomical Society Celestial Events 4 c/o Matt McCullar 5801 Trail Lake Drive Sky Chart 5 Fort Worth, TX 76133 Moon Phase Calendar 6 Web Site: http://www.fortworthastro.org Facebook: http://tinyurl.com/3eutb22 Lunar Occultations/Conjs 7 Twitter: http://twitter.com/ftwastro Yahoo! eGroup (members only): http://tinyurl.com/7qu5vkn Mercury/Venus Chart 8 Officers (2014-2015): Mars/Minor Planets Charts 9 President – Bruce Cowles, [email protected] Jupiter Charts 10 Vice President – Russ Boatwright, [email protected] Sec/Tres – Michelle Theisen, [email protected] Planet Vis & ISS Passes 11 Board Members: CSAC Event Update 12 2014-2016 Mike Langohr Young Astronomer News 12 Tree Oppermann ‘66 Leonids Remembered 13 2013-2015 Bill Nichols Cloudy Night Library 15 Jim Craft Cover Photo: Monthly AL Observing Club 17 Composite image taken by FWAS mem- bers: Left to right, from top to bottom— Constellation of the Month 18 Laura Cowles, Mike Ahner, Brian Wortham, Constellation Mythology 19 Shawn Kirchdorfer, Mark Wainright, Phil Stage, Patrick McMahon, Dennis Webb, Ben Prior Club Meeting Minutes 20 Hudgens, Shawn Kirchdorfer, John McCrea, and Chris Mlodnicki General Club Information 21 That’s A Fact 21 Observing Site Reminders: Be careful with fire, mind all local burn bans! Full Moon Name 21 Dark Site Usage Requirements (ALL MEMBERS): FWAS Foto Files 22 Maintain Dark-Sky Etiquette (http://tinyurl.com/75hjajy) Turn out your headlights at the gate! Sign the logbook (in camo-painted storage shed.
    [Show full text]
  • Abstract Neutral Gas Outflows and Inflows in Local AGN & High-Z Lyman-Α Emitters in COSMOS Hannah Bowen Krug, Doctor Of
    Abstract Title of dissertation: Neutral Gas Outflows and Inflows in Local AGN & High-z Lyman-α Emitters in COSMOS Hannah Bowen Krug, Doctor of Philosophy, 2013 Dissertation directed by: Professor Sylvain Veilleux Department of Astronomy This thesis is composed of two parts: (1) a search for neutral gas outflows and inflows in local active galactic nuclei (AGN) and ultraluminous infrared galax- ies (ULIRGs), and (2) a deep and wide imaging search for high-redshift Lyman-α emitters (LAEs). In the first part, we utilize the R-C spectrograph on the Mayall 4m telescope at Kitt Peak National Observatory (KPNO) to look for Na I D ab- sorption. Galactic outflows are thought to play a major role in galactic feedback and evolution, and previous studies of neutral gas have shown that galactic winds occur in most galaxies with high infrared (IR) luminosities. However, in composite systems where a starburst coexists with an active galactic nucleus (AGN), it is un- clear whether the starburst or the AGN is driving the outflows. This thesis attempts to answer that question by looking at samples of Seyfert galaxies, Palomar-Green quasistellar objects (PG QSOs), and ULIRGs. We first describe the results from a search for Na I D outflows in 35 IR- faint Seyferts. We find that the outflow detection rates for IR-faint Seyferts are substantially lower than those of IR-luminous Seyferts. The outflow kinematics of Seyfert 2s resemble those of starburst galaxies, while the outflow velocities in Seyfert 1s are significantly larger. Taken together, these results suggest that the AGN does not play a significant role in driving the outflows in most Seyferts, except the high- velocity outflows seen in Seyfert 1s.
    [Show full text]
  • An Atlas of Calcium Triplet Spectra of Active Galaxies 3
    Mon. Not. R. Astron. Soc. 000, 000–000 (0000) Printed 1 December 2018 (MN LATEX style file v2.2) An atlas of Calcium triplet spectra of active galaxies A. Garcia-Rissmann1⋆, L. R. Vega1,2†, N. V. Asari1‡, R. Cid Fernandes1§, H. Schmitt3,4¶, R. M. Gonz´alez Delgado5k, T. Storchi-Bergmann6⋆⋆ 1 Depto. de F´ısica - CFM - Universidade Federal de Santa Catarina, C.P. 476, 88040-900, Florian´opolis, SC, Brazil 2 Observatorio Astron´omico de C´ordoba, Laprida 854, 5000, C´ordoba, Argentina 3 Remote Sensing Division, Code 7210, Naval Research Laboratory, 4555 Overlook Avenue, SW, Washington, DC 20375 4 Interferometric Inc., 14120 Parke Long Court, 103, Chantilly, VA20151 5 Instituto de Astrof´ısica de Andaluc´ıa (CSIC), P.O. Box 3004, 18080 Granada, Spain 6 Instituto de F´ısica, Universidade Federal do Rio Grande do Sul, C.P. 15001, 91501-970, Porto Alegre, RS, Brazil 1 December 2018 ABSTRACT We present a spectroscopic atlas of active galactic nuclei covering the region around the λλ8498, 8542, 8662 Calcium triplet (CaT). The sample comprises 78 ob- jects, divided into 43 Seyfert 2s, 26 Seyfert 1s, 3 Starburst and 6 normal galaxies. The spectra pertain to the inner ∼ 300 pc in radius, and thus sample the central kine- matics and stellar populations of active galaxies. The data are used to measure stellar velocity dispersions (σ⋆) both with cross-correlation and direct fitting methods. These measurements are found to be in good agreement with each-other and with those in previous studies for objects in common. The CaT equivalent width is also measured.
    [Show full text]
  • The Large Scale Distribution of Radio Continuum in Ε and So Galaxies
    THE LARGE SCALE DISTRIBUTION OF RADIO CONTINUUM IN Ε AND SO GALAXIES R.D. Ekers, Kapteyn Astronomical Institute, University of Groningen If we look at the radio properties of the nearby ellipticals we find a situation considerably different from that just described by van der Kruit for the spiral galaxies. For example NGC 5128 (Cen A), the nearest giant elliptical galaxy, is a thousand times more powerful a radio source than the brightest spiral galaxies and furthermore its radio emission comes from a multiple lobed radio structure which bears no resemblance to the optical light distribution (e.g. Ekers, 1975). The other radio emitting elliptical galaxies in our neighbourhood, NGC 1316 (Fornax A), IC 4296 (1333-33), have similar morphology. A question which then arises is whether at lower levels we can detect radio emission coming from the optical image of the elliptical galaxies and which may be more closely related to the kind of emission seen in the spiral galaxies. Since elliptical galaxies are less numerous than spiral galaxies we have to search out to the Virgo cluster to obtain a good sample. Some results from a Westerbork map of the central region of the Virgo cluster at 1.4 GHz (Kotanyi and Ekers, in preparation) is given in the Table. Radio Emission from Galaxies in the core of the Virgo Cluster Name Hubble m Flux density NGC Type Ρ (JO"29 W m-2 Hz-1) 4374 El 10.8 6200 3C 272.1 4388 Sc 12.2 140 4402 Sd 13.6 60 4406 E3 10.9 < 4 4425 SO 13.3 < 4 4435 SO 1 1.9 < 5 4438 S pec 12.0 150 This result is typical for spiral and elliptical galaxies and illustrates the different properties quite well.
    [Show full text]
  • 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,
    [Show full text]