Hostname: page-component-586b7cd67f-l7hp2 Total loading time: 0 Render date: 2024-11-23T07:02:37.776Z Has data issue: false hasContentIssue false
  • English
  • Français

The Nuclear Disk of NGC4261: HST Images and WHT Spectra

Published online by Cambridge University Press:  19 July 2016

Laura Ferrarese ,
Holland C. Ford ,
Walter Jaffe ,
Frank van den Bosch  and
Robert W. O'Connell
Laura Ferrarese
Affiliation:
Johns Hopkins University and Space Telescope Science Institute
Holland C. Ford
Affiliation:
Johns Hopkins University and Space Telescope Science Institute
Walter Jaffe
Affiliation:
Leiden Observatory
Frank van den Bosch
Affiliation:
Leiden Observatory
Robert W. O'Connell
Affiliation:
University of Virginia

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The properties of the nuclear region of the elliptical galaxy NGC4261 (=3C270), the second brightest radio source in the Virgo cluster, have been studied using high resolution HST images and La Palma WHT spectra.

Type
Poster Contributions: Disks Structure and Emission
Information
Symposium - International Astronomical Union , Volume 159: Multi-Wavelength Continuum Emission of AGN , 1994 , pp. 479
Copyright
Copyright © Kluwer 1994 

References

1. Jaffe, W. et al. 1993, Nature, 364, 312 and references therein.CrossRefGoogle Scholar