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Gas, Dust and Radio Emission in Elliptical Galaxies
Published online by Cambridge University Press: 04 August 2017
Abstract
CCD data are used to compare the isophotes, colour and dust-content of radio (1021<P5GHz<1024WHz-1, HO = 75kms-1Mpc-1) and radio-quiet ellipticals. Radio ellipticals are round but not spheroidal, reddened and occasionally have disturbed dust lanes. X-ray emission correlates with both radio emission and shape. Detailed investigations of dust in NGC 1316 reveal a possible nuclear gas disc orthogonal to the radio jet.
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- Posters
- Information
- Symposium - International Astronomical Union , Volume 127: Structure and Dynamics of Elliptical Galaxies , 1987 , pp. 425 - 426
- Copyright
- Copyright © Reidel 1987