Integral Field Unit Spectroscopy of 10 Early Type Galactic Nuclei: I-Principal
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198 7Apj. . .312L. .11J the Astrophysical Journal, 312:L11-L15
.11J The Astrophysical Journal, 312:L11-L15,1987 January 1 .312L. © 1987. The American Astronomical Society. All rights reserved. Printed in U.S.A. 7ApJ. 198 INTERSTELLAR DUST IN SHAPLEY-AMES ELLIPTICAL GALAXIES M. Jura and D. W. Kim Department of Astronomy, University of California, Los Angeles AND G. R. Knapp and P. Guhathakurta Princeton University Observatory Received 1986 August 11; accepted 1986 September 30 ABSTRACT We have co-added the IRAS survey data at the positions of the brightest elliptical galaxies in the Revised Shapley-Ames Catalog to increase the sensitivity over that of the IRAS Point Source Catalog. More than half of 7 8 the galaxies (with Bj< \\ mag) are detected at 100 /xm with flux levels indicating, typically, 10 or 10 M0 of cold interstellar matter. The presence of cold gas in ellipticals thus appears to be the rule rather than the exception. Subject headings: galaxies: general — infrared: sources I. INTRODUCTION infrared emission from the elliptical galaxy in the line of sight. The traditional view of early-type galaxies is that they are Our criteria for a real detection are as follows: essentially free of interstellar matter. However, with advances 1. The optical position of the galaxy and the position of the in instrumental sensitivity, it has become possible to observe IRAS source agree to better than V. (The agreement is usually 21 cm emission (Knapp, Turner, and Cunniffe 1985; Wardle much better than T.) and Knapp 1986), optical dust patches (Sadler and Gerhard 2. The flux is at least 3 times the r.m.s. noise. -
Stripped Elliptical Galaxies As Probes of Icm Physics. Ii
The Astrophysical Journal, 806:104 (15pp), 2015 June 10 doi:10.1088/0004-637X/806/1/104 © 2015. The American Astronomical Society. All rights reserved. STRIPPED ELLIPTICAL GALAXIES AS PROBES OF ICM PHYSICS. II. STIRRED, BUT MIXED? VISCOUS AND INVISCID GAS STRIPPING OF THE VIRGO ELLIPTICAL M89 E. Roediger1,2,5, R. P. Kraft2, P. E. J. Nulsen2, W. R. Forman2, M. Machacek2, S. Randall2, C. Jones2, E. Churazov3, and R. Kokotanekova4 1 Hamburger Sternwarte, Universität Hamburg, Gojensbergsweg 112, D-21029 Hamburg, Germany; [email protected] 2 Harvard/Smithsonian Center for Astrophysics, 60 Garden Street MS-4, Cambridge, MA 02138, USA 3 MPI für Astrophysik, Karl-Schwarzschild-Str. 1, Garching D-85741, Germany 4 AstroMundus Master Programme, University of Innsbruck, Technikerstr. 25/8, 6020 Innsbruck, Austria Received 2014 September 18; accepted 2015 March 29; published 2015 June 10 ABSTRACT Elliptical galaxies moving through the intracluster medium (ICM) are progressively stripped of their gaseous atmospheres. X-ray observations reveal the structure of galactic tails, wakes, and the interface between the galactic gas and the ICM. This fine-structure depends on dynamic conditions (galaxy potential, initial gas contents, orbit in the host cluster), orbital stage (early infall, pre-/post-pericenter passage), as well as on the still ill-constrained ICM plasma properties (thermal conductivity, viscosity, magnetic field structure). Paper I describes flow patterns and stages of inviscid gas stripping. Here we study the effect of a Spitzer-like temperature dependent viscosity corresponding to Reynolds numbers, Re, of 50–5000 with respect to the ICM flow around the remnant atmosphere. Global flow patterns are independent of viscosity in this Reynolds number range. -
The Globular Cluster System of NGC 1399
Astronomy & Astrophysics manuscript no. sch1399 c ESO 2018 August 28, 2018 The globular cluster system of NGC 1399 ⋆,⋆⋆ V. dynamics of the cluster system out to 80 kpc Y. Schuberth1,2, T. Richtler2, M. Hilker3, B. Dirsch2, L. P. Bassino4, A. J. Romanowsky5,2, and L. Infante6 1 Argelander-Institut f¨ur Astronomie, Universit¨at Bonn, Auf dem H¨ugel 71, D-53121 Bonn, Germany 2 Universidad de Concepci´on, Departamento de Astronomia, Casilla 160-C, Concepci´on, Chile 3 European Southern Observatory, Karl-Schwarzschild-Str. 2, D-85748 Garching, Germany 4 Facultad de Ciencias Astron´omicas y Geof´ısicas, Universidad Nacional de La Plata, Paseo del Bosque S/N, 1900–La Plata, Argentina; and Instituto de Astrof´ısica de La Plata (CCT La Plata – CONICET – UNLP) 5 UCO/Lick Observatory, University of California, Santa Cruz, CA 95064, USA 6 Departamento de Astronom´ıa y Astrof´ısica, Pontificia Universidad Cat´olica de Chile, Casilla 306, Santiago 22, Chile Received 14 May, 2009; accepted 16 October, 2009 ABSTRACT Globular clusters (GCs) are tracers of the gravitational potential of their host galaxies. Moreover, their kinematic properties may provide clues for understanding the formation of GC systems and their host galaxies. We use the largest set of GC velocities obtained so far of any elliptical galaxy to revise and extend the previous investigations (Richtler et al. 2004) of the dynamics of NGC 1399, the central dominant galaxy of the nearby Fornax cluster of galaxies. The GC velocities are used to study the kinematics, their relation with population properties, and the dark matter halo of NGC 1399. -
Aspects of Supermassive Black Hole Growth in Nearby Active Galactic Nuclei Davide Lena
Rochester Institute of Technology RIT Scholar Works Theses Thesis/Dissertation Collections 4-2015 Aspects of Supermassive Black Hole Growth in Nearby Active Galactic Nuclei Davide Lena Follow this and additional works at: http://scholarworks.rit.edu/theses Recommended Citation Lena, Davide, "Aspects of Supermassive Black Hole Growth in Nearby Active Galactic Nuclei" (2015). Thesis. Rochester Institute of Technology. Accessed from This Dissertation is brought to you for free and open access by the Thesis/Dissertation Collections at RIT Scholar Works. It has been accepted for inclusion in Theses by an authorized administrator of RIT Scholar Works. For more information, please contact [email protected]. Aspects of Supermassive Black Hole Growth in Nearby Active Galactic Nuclei A Search for Recoiling Supermassive Black Holes Gas Kinematics in the Circumnuclear Region of Two Seyfert Galaxies Davide Lena A dissertation submitted in partial fulfillment of the requirements for the degree of Ph.D. in Astrophysical Sciences and Technology in the College of Science, School of Physics and Astronomy Rochester Institute of Technology © D. Lena April, 2015 Cover image: flux map for the [NII]λ6583 emission line in the nuclear region of the Seyfert galaxy NGC 1386. The map was derived from integral field observations performed with the Gemini Multi Object Spectrograph on the Gemini-South Observatory. Certificate of Approval Astrophysical Sciences and Technologies R·I·T College of Science Rochester, NY, USA The Ph.D. Dissertation of DAVIDE LENA has been approved by the undersigned members of the dissertation committee as satisfactory for the degree of Doctor of Philosophy in Astrophysical Sciences and Technology. -
115 Abell Galaxy Cluster # 373
WINTER Medium-scope challenges 271 # # 115 Abell Galaxy Cluster # 373 Target Type RA Dec. Constellation Magnitude Size Chart AGCS 373 Galaxy cluster 03 38.5 –35 27.0 Fornax – 180 ′ 5.22 Chart 5.22 Abell Galaxy Cluster (South) 373 272 Cosmic Challenge WINTER Nestled in the southeast corner of the dim early winter western suburbs. Deep photographs reveal that NGC constellation Fornax, adjacent to the distinctive triangle 1316 contains many dust clouds and is surrounded by a formed by 6th-magnitude Chi-1 ( 1), Chi-2 ( 2), and complex envelope of faint material, several loops of Chi-3 ( 3) Fornacis, is an attractive cluster of galaxies which appear to engulf a smaller galaxy, NGC 1317, 6 ′ known as Abell Galaxy Cluster – Southern Supplement to the north. Astronomers consider this to be a case of (AGCS) 373. In addition to his research that led to the galactic cannibalism, with the larger NGC 1316 discovery of more than 80 new planetary nebulae in the devouring its smaller companion. The merger is further 1950s, George Abell also examined the overall structure signaled by strong radio emissions being telegraphed of the universe. He did so by studying and cataloging from the scene. 2,712 galaxy clusters that had been captured on the In my 8-inch reflector, NGC 1316 appears as a then-new National Geographic Society–Palomar bright, slightly oval disk with a distinctly brighter Observatory Sky Survey taken with the 48-inch Samuel nucleus. NGC 1317, about 12th magnitude and 2 ′ Oschin Schmidt camera at Palomar Observatory. In across, is visible in a 6-inch scope, although averted 1958, he published the results of his study as a paper vision may be needed to pick it out. -
CHEERS): Constraints on Turbulence
A&A 575, A38 (2015) Astronomy DOI: 10.1051/0004-6361/201425278 & c ESO 2015 Astrophysics Chemical Enrichment RGS cluster Sample (CHEERS): Constraints on turbulence Ciro Pinto1, Jeremy S. Sanders2, Norbert Werner3,4, Jelle de Plaa5, Andrew C. Fabian1, Yu-Ying Zhang6, Jelle S. Kaastra5, Alexis Finoguenov7, and Jussi Ahoranta7 1 Institute of Astronomy, Madingley Road, CB3 0HA Cambridge, UK e-mail: [email protected]. 2 Max-Planck-Institut fur extraterrestrische Physik, Giessenbachstrasse 1, 85748 Garching, Germany 3 Kavli Institute for Particle Astrophysics and Cosmology, Stanford University, 452 Lomita Mall, Stanford, CA 94305-4085, USA 4 Department of Physics, Stanford University, 382 via Pueblo Mall, Stanford, CA 94305-4060, USA 5 SRON Netherlands Institute for Space Research, Sorbonnelaan 2, 3584 CA Utrecht, The Netherlands 6 Argelander-Institut für Astronomie, Universität Bonn, Auf dem Hügel 71, 53121 Bonn, Germany 7 Department of Physics, University of Helsinki, 00014 Helsinki, Finland Received 5 November 2014 / Accepted 24 December 2014 ABSTRACT Context. Feedback from active galactic nuclei, galactic mergers, and sloshing are thought to give rise to turbulence, which may prevent cooling in clusters. Aims. We aim to measure the turbulence in clusters of galaxies and compare the measurements to some of their structural and evolutionary properties. Methods. It is possible to measure the turbulence of the hot gas in clusters by estimating the velocity widths of their X-ray emission lines. The Reflection Grating Spectrometers aboard XMM-Newton are currently the only instruments provided with sufficient effective area and spectral resolution in this energy domain. We benefited from excellent 1.6 Ms new data provided by the Chemical Enrichment RGS cluster Sample (CHEERS) project. -
Professor Catriona Macleod
RRR | Cover 2015 v2 11/9/16 10:17 AM Page 1 C M Y CM MY CY CMY K Composite RRR 2015 | Features 11/12/16 1:36 PM Page 1 C M Y CM MY CY CMY K RHODES UNIVERSITY RESEARCH REPORT A publication of the Rhodes University Research Office, compiled and edited by Tarryn Gillitt, Busi Goba, Patricia Jacob, Jill Macgregor and Jaine Roberts Design & Layout: Sally Dore Research Office Director: Jaine Roberts [email protected] Tel: +27 (46) 603 8756/7572 www.ru.ac.za Cover: Rhodes University researchers Pam Maseko, Nomalanga Mkhize, Heila Lotz-Sisitka, Ruth Simbao, Anthea Garman and Catriona Macleod Cover Photos: Paul Greenway/www.3pphotography.com RESEARCH REPORT 2015 Composite RRR 2015 | Features 11/12/16 1:36 PM Page 2 C M Y CM MY CY CMY K CONTENTS 01 FOREWORD Dr Sizwe Mabizela, Vice-Chancellor 03 INTRODUCTION Dr Peter Clayton, Deputy Vice-Chancellor: Research & Development 05 TOP 30 RESEARCHERS 06 PHD GRADUATES 11 VICE-CHANCELLOR’S BOOK AWARD Professor Anthea Garman 13 VICE-CHANCELLOR’S DISTINGUISHED SENIOR RESEARCH AWARD Professor Catriona Macleod 15 VICE-CHANCELLOR’S DISTINGUISHED RESEARCH AWARD Dr Adrienne Edkins 17 SARChI CHAIRS Professor Heila Lotz-Sisitka, Professor Ruth Simbao and Dr Adrienne Edkins 23 AFRICAN LANGUAGES, SCHOOL OF LANGUAGES AND LITERATURE Associate Professor Pamela Maseko 25 DEPARTMENT OF HISTORY Dr Nomalanga Mkhize RESEARCH REPORT 2015 Composite RRR 2015 | Features 11/12/16 1:34 PM Page 3 C M Y CM MY CY CMY K RHODES RESEARCH 2015 RESEARCH REPORT DEPARTMENT PUBLICATIONS AFFILIATES, INSTITUTES AND 28 Publications from the Vice-Chancellorate -
The Low-Metallicity Picture A
Linking dust emission to fundamental properties in galaxies: the low-metallicity picture A. Rémy-Ruyer, S. C. Madden, F. Galliano, V. Lebouteiller, M. Baes, G. J. Bendo, A. Boselli, L. Ciesla, D. Cormier, A. Cooray, et al. To cite this version: A. Rémy-Ruyer, S. C. Madden, F. Galliano, V. Lebouteiller, M. Baes, et al.. Linking dust emission to fundamental properties in galaxies: the low-metallicity picture. Astronomy and Astrophysics - A&A, EDP Sciences, 2015, 582, pp.A121. 10.1051/0004-6361/201526067. cea-01383748 HAL Id: cea-01383748 https://hal-cea.archives-ouvertes.fr/cea-01383748 Submitted on 19 Oct 2016 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. A&A 582, A121 (2015) Astronomy DOI: 10.1051/0004-6361/201526067 & c ESO 2015 Astrophysics Linking dust emission to fundamental properties in galaxies: the low-metallicity picture? A. Rémy-Ruyer1;2, S. C. Madden2, F. Galliano2, V. Lebouteiller2, M. Baes3, G. J. Bendo4, A. Boselli5, L. Ciesla6, D. Cormier7, A. Cooray8, L. Cortese9, I. De Looze3;10, V. Doublier-Pritchard11, M. Galametz12, A. P. Jones1, O. Ł. Karczewski13, N. Lu14, and L. Spinoglio15 1 Institut d’Astrophysique Spatiale, CNRS, UMR 8617, 91405 Orsay, France e-mail: [email protected]; [email protected] 2 Laboratoire AIM, CEA/IRFU/Service d’Astrophysique, Université Paris Diderot, Bât. -
Probing the Physics of Narrow Line Regions in Active Galaxies II: the Siding Spring Southern Seyfert Spectroscopic Snapshot Survey (S7)
Probing the Physics of Narrow Line Regions in Active Galaxies II: The Siding Spring Southern Seyfert Spectroscopic Snapshot Survey (S7) Michael A. Dopita1,2, Prajval Shastri3, Rebecca Davies1, Lisa Kewley1,4, Elise Hampton1, Julia Scharw¨achter5, Ralph Sutherland1, Preeti Kharb3, Jessy Jose3, Harish Bhatt3, S. Ramya 3, Chichuan Jin6, Julie Banfield7, Ingyin Zaw8, St´ephanie Juneau9, Bethan James10 & Shweta Srivastava11 [email protected] ABSTRACT Here we describe the Siding Spring Southern Seyfert Spectroscopic Snapshot Survey (S7) and present results on 64 galaxies drawn from the first data release. The S7 uses the Wide Field Spectrograph (WiFeS) mounted on the ANU 2.3m telescope located at the Siding Spring Observatory to deliver an integral field of 38×25 arcsec at a spectral resolution of R = 7000 in the red (530−710nm), and R = 3000 in the blue (340 − 560nm). From these data cubes we have extracted the Narrow Line Region (NLR) spectra from a 4 arc sec aperture centred on the nucleus. We also determine the Hβ and [O III] λ5007 fluxes in the narrow lines, the nuclear reddening, the reddening-corrected relative intensities of the observed emission lines, and the Hβ and [O III] λ5007 luminosities determined 1RSAA, Australian National University, Cotter Road, Weston Creek, ACT 2611, Australia 2Astronomy Department, King Abdulaziz University, P.O. Box 80203, Jeddah, Saudi Arabia 3Indian Institute of Astrophysics, Koramangala 2B Block, Bangalore 560034, India 4Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI, USA 5LERMA, Observatoire de Paris, CNRS, UMR 8112, 61 Avenue de l’Observatoire, 75014, Paris, France 6Qian Xuesen Laboratory for Space Technology, Beijing, China 7CSIRO Astronomy & Space Science, P.O. -
ALABAMA University Libraries
THE UNIVERSITY OF ALABAMA University Libraries O VI In Elliptical Galaxies: Indicators of Cooling Flows Joel N. Bregman – University of Michigan Eric D. Miller – MIT Alex E. Athey – Carnegie Institution of Washington Jimmy A. Irwin – University of Michigan Deposited 09/13/2018 Citation of published version: Bregman, J., Miller, E., Athey, A., Irwin, J. (2005): O VI In Elliptical Galaxies: Indicators of Cooling Flows The Astrophysical Journal, 635(2). DOI: 10.1086/497421 © 2005. The American Astronomical Society. All rights reserved. Printed in U.S.A. The Astrophysical Journal, 635:1031–1043, 2005 December 20 # 2005. The American Astronomical Society. All rights reserved. Printed in U.S.A. O vi IN ELLIPTICAL GALAXIES: INDICATORS OF COOLING FLOWS Joel N. Bregman Department of Astronomy, University of Michigan, Ann Arbor, MI 48109; [email protected] Eric D. Miller Kavli Institute for Astrophysics and Space Science, MIT, Cambridge, MA 02139; [email protected] Alex E. Athey The Observatories, Carnegie Institution of Washington, Pasadena, CA 91101; [email protected] and Jimmy A. Irwin Department of Astronomy, University of Michigan, Ann Arbor, MI 48109; [email protected] Received 2005 April 25; accepted 2005 August 23 ABSTRACT Early-type galaxies often contain a hot X-ray–emitting interstellar medium [(3 8) ; 106 K] with an apparent radiative cooling time much less than a Hubble time. If unopposed by a heating mechanism, the gas will radiatively 4 À1 cool to temperatures P10 K at a rate proportional to LX /TX , typically 0.03–1 M yr . We can test whether gas is cooling through the 3 ; 105 K range by observing the O vi doublet, whose luminosity is proportional to the cooling rate. -
The Fornax Cluster VLT Spectroscopic Survey II &Ndash
University of Groningen The Fornax Cluster VLT Spectroscopic Survey II - Planetary Nebulae kinematics within 200 kpc of the cluster core Spiniello, C.; Napolitano, N. R.; Arnaboldi, M.; Tortora, C.; Coccato, L.; Capaccioli, M.; Gerhard, O.; Iodice, E.; Spavone, M.; Cantiello, M. Published in: Monthly Notices of the Royal Astronomical Society DOI: 10.1093/mnras/sty663 IMPORTANT NOTE: You are advised to consult the publisher's version (publisher's PDF) if you wish to cite from it. Please check the document version below. Document Version Publisher's PDF, also known as Version of record Publication date: 2018 Link to publication in University of Groningen/UMCG research database Citation for published version (APA): Spiniello, C., Napolitano, N. R., Arnaboldi, M., Tortora, C., Coccato, L., Capaccioli, M., ... Schipani, P. (2018). The Fornax Cluster VLT Spectroscopic Survey II - Planetary Nebulae kinematics within 200 kpc of the cluster core. Monthly Notices of the Royal Astronomical Society, 477(2), 1867-1879. https://doi.org/10.1093/mnras/sty663 Copyright Other than for strictly personal use, it is not permitted to download or to forward/distribute the text or part of it without the consent of the author(s) and/or copyright holder(s), unless the work is under an open content license (like Creative Commons). Take-down policy If you believe that this document breaches copyright please contact us providing details, and we will remove access to the work immediately and investigate your claim. Downloaded from the University of Groningen/UMCG research database (Pure): http://www.rug.nl/research/portal. For technical reasons the number of authors shown on this cover page is limited to 10 maximum. -
The Globular Cluster System of NGC 4526
The globular cluster system of NGC 4526 Leonie Chevalier Presented in fulfillment of the requirements of the degree of Masters by Research { Faculty of Science and Technology Swinburne University i You couldn't put off the inevitable. Because sooner or later, you reached the place when the inevitable just went and waited - Terry Pratchett, Small Gods ii Abstract With ages up to ∼ 12.8 Gyr, globular clusters (GCs) are some of the oldest objects we observe in galaxies and are thought to preserve their parent galaxy's chemo-dynamical properties at the time of their formation. A single galaxy can have tens of thousands of GCs associated with it. Globular cluster systems have long been thought to be a useful tool for constraining galaxy formation scenarios and even to infer a galaxy's individual formation history. More recently GCs have been used to infer dark matter masses of galaxies. This thesis focuses on the GC system of the lenticular galaxy NGC 4526. We used Subaru imaging to study the system's full extent and infer the total number of GCs as well as the substructure in the GC system. Additionally we used the DEIMOS spectrograph on the Keck telescope to obtain radial velocities for 106 GCs to be used in studying the dark matter content of NGC 4526. The combination of multiband photometric data in combination with the spectroscopic data gained by DEIMOS is a significant improvement on existing data sets that only partially imaged the GC system. To put our findings into a broader context we compared NGC 4526 to the results of 26 other elliptical and lenticular galaxies (and their GC systems) from existing literature.