Volume 383, Number 1, FebruaryIII 2002
|Page(s)||98 - 103|
|Section||Cosmology (including clusters of galaxies)|
|Published online||15 February 2002|
Radio observations of the circumnuclear ring in NGC 6951
Department of Physics, Queen's University, Kingston, Ontario, K7L 3N6, Canada
2 Jodrell Bank Observatory, University of Manchester, Macclesfield, Cheshire SK11 9DL, UK
3 National Centre for Radio Astrophysics, Tata Institute of Fundamental Research, Post Bag No. 3, Ganeshkhind, Pune 411 007, India
4 St. Stephen's College, University of Delhi, Delhi 110 007, India
5 Onsala Space Observatory, 43992 Onsala, Sweden
6 Nobeyama Radio Observatory, Minamimaki, Minamisaku, Nagano 384-1305, Japan
7 Institute of Astronomy, University of Tokyo, Osawa, Mitaka, Tokyo 181-0015, Japan
Corresponding author: D. J. Saikia, email@example.com
Accepted: 3 December 2001
We present sensitive, high-resolution radio observations of the circumnuclear region of the barred spiral galaxy NGC 6951. These observations reveal a ring of radio emission with many discrete components and a marginally resolved nuclear component. We compare the radio ring with observations at other wavelengths, and discuss the nature of the compact radio components.
Key words: galaxies: active / galaxies: individual: NGC 6951 / galaxies: nuclei / galaxies: spiral / radio continuum: galaxies
© ESO, 2002
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