Published by
EDP Sciences
EDP Sciences Journals List
Subscriber Authentication Point
Home All issues Volume 502/ 2 Article
Issue A&A
Volume 502, Number 2, August I 2009
Page(s) L5 - L8
Section Letters
DOI http://dx.doi.org/10.1051/0004-6361/200912624
Published online 02 July 2009

A&A 502, L5-L8 (2009)
DOI: 10.1051/0004-6361/200912624

Letter

Uncovering the kiloparsec-scale stellar ring of NGC 5128

J. T. Kainulainen1, 2, J. F. Alves3, Y. Beletsky4, J. Ascenso5, J. M. Kainulainen6, A. Amorim7, J. Lima7, R. Marques8, A. Moitinho7, J. Pinhão8, J. Rebordão9, and F. D. Santos7

1  Observatory, PO Box 14, 00014 Univ. of Helsinki, Finland
    e-mail: jtkainul@mpia-hd.mpg.de
2  TKK/Metsähovi Radio Observatory, Metsähovintie 114, 02540 Kylmälä, Finland
3  Calar Alto Observatory, Centro Astronómico Hispano, Alemán, C/q Jesús Durbán Remón 2-2, 04004 Almeria, Spain
4  European Southern Observatory (ESO), Alonso de Cordova 3107, Santiago, Chile
5  Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA
6  TKK/Department of Radio Science and Engineering, PO Box 3000, 02015 TKK, Finland
7  SIM-IDL, Faculdade de Ciências da Universidade de Lisboa, Ed. C8. Campo Grande 1749-016 Lisbon, Portugal
8  LIP-Coimbra, Department of Physics, University of Coimbra, 3004-516 Coimbra, Portugal
9  INETI, Estrada da Portela, Zambujal-Alfragide, Apartado 7586, 2720-866 Amadora, Portugal

Received 3 June 2009 / Accepted 13 June 2009

Abstract
We reveal the stellar light emerging from the kiloparsec-scale, ring-like structure of the NGC 5128 (Centaurus A) galaxy in unprecedented detail. We use arcsecond-scale resolution near infrared images to create a “dust-free” view of the central region of the galaxy, which we then use to quantify the shape of the revealed structure. At the resolution of the data, the structure contains several hundreds of discreet, point-like or slightly elongated sources. The typical extinction-corrected surface brightness of the structure is $K_{\rm S} \approx 16.5$ mag/arcsec2, and we estimate the total near infrared luminosity of the structure to be $M \approx -21$ mag. We use diffraction limited ($\it FWHM$ resolution of  ${\approx}0.1^{\prime\prime}$, or 1.6 pc) near infrared data taken with the NACO instrument on the VLT to show that the structure decomposes into thousands of separate, mostly point-like sources. According to the tentative photometry, the most luminous sources have $M_{K} \approx -12$ mag, making them red supergiants or relatively low-mass star clusters. We also discuss the large-scale geometry implied by the reddening signatures of dust in our near infrared images.


Key words: ISM: dust, extinction -- galaxies: individual: NGC 5128 -- galaxies: ISM -- galaxies: structure -- infrared: galaxies



© ESO 2009

What is OpenURL?

The OpenURL standard is a protocol for transmission of metadata describing the resource that you wish to access. An OpenURL link contains article metadata and directs it to the OpenURL server of your choice. The OpenURL server can provide access to the resource and also offer complementary services (specific search engine, export of references...). The OpenURL link can be generated by different means.
  • If your librarian has set up your subscription with an OpenURL resolver, OpenURL links appear automatically on the abstract pages.
  • You can define your own OpenURL resolver with your EDPS Account. In this case your choice will be given priority over that of your library.
  • You can use an add-on for your browser (Firefox or I.E.) to display OpenURL links on a page (see http://www.openly.com/openurlref/). You should disable this module if you wish to use the OpenURL server that you or your library have defined.