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HST Observations of Jets and Radio Lobes

Published online by Cambridge University Press:  25 May 2016

Philippe Crane
Philippe Crane*
Affiliation:
European Southern Observatory Karl Schwarzschildstraße 2 D85748 Garching Germany

Extract

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The Hubble Space Telescope has proved to be remarkably useful for discovering and for studying the optical counterparts of radio lobes and radio jets. Since much of the structure seen in the radio is found on subarcsecond scales, it is not surprising that HST, with it's improved resolution relative to ground based observations, would be a major contributor to this field of research. This paper reports briefly on some of these successes, and refers to more detailed descriptions in the literature.

Type
Relation between Radio and Other Wavelenghts
Information
Symposium - International Astronomical Union , Volume 175: Extragalactic Radio Sources , 1996 , pp. 201 - 202
Copyright
Copyright © Kluwer 1996 

References

1. Röser, H.J., and Meisenheimer, K., (1987) Ap. J. 314, 70.CrossRefGoogle Scholar
2. Thomson, R.C., Crane, P., and Mackay, C.D., (1995) Ap.J. Letters , 446, L93.Google Scholar
3. Crane, P., Peletier, R., et al., (1993) Ap.J. Letters , 402, L37.Google Scholar
4. Crane, P., Pedlar, A., et al.,(1996) in preparation.Google Scholar
5. Perley, R., Bridle, A.H., and Willis, A.G., (1984) Ap. J. Suppl. , 54,291.Google Scholar
6. Crane, P., 1993 in Jets in Extragalactic Radio Sources , edited by, Röser, H.J. and Meisenheimer, K., (Berlin: Spinger)pp 223.Google Scholar
7. Wyckoff, S., et al.(1983) Ap. J. 265,43.CrossRefGoogle Scholar
8. Crane, P., and Stiavelli, M.,(1992) MNRAS 257,17P.Google Scholar