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HST/STIS Spectroscopy of CSS Sources: Kinematics and Ionisation of the Aligned Nebulae

Published online by Cambridge University Press:  05 March 2013

A. Labiano
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore MD, USA, 21218. [email protected], [email protected], [email protected], [email protected] Kapteyn Astronomical Institute, PO Box 800, Groningen, Holland, 9700 AV. [email protected], [email protected]
C. P. O'Dea
Affiliation:
Western Kentucky University, 1 Big Red Way, Bowling Green KY, USA 42101-3576. [email protected]
R. Gelderman
Affiliation:
Lawrence Livermore National Laboratory, 7000 East Avenue, Livermore CA, USA 94550-9234. [email protected]
W. H. de Vries
Affiliation:
University of Hertfordshire, College Lane, Hatfield Herts, UK AL10 9AB. [email protected]
D. J. Axon
Affiliation:
University of Hertfordshire, College Lane, Hatfield Herts, UK AL10 9AB. [email protected]
P. D. Barthel
Affiliation:
Kapteyn Astronomical Institute, PO Box 800, Groningen, Holland, 9700 AV. [email protected], [email protected]
S. A. Baum
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore MD, USA, 21218. [email protected], [email protected], [email protected], [email protected]
A. Capetti
Affiliation:
Osservatorio Astronomico di Torino, Via Osservatorio 20, Pino Torinesse (TO), Italy 10025. [email protected]
R. Fanti
Affiliation:
Instituto di Radioastronomia del CNR, Via P. Gobetti, 101, Bologna, Italy 40129. [email protected]
A. M. Koekemoer
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore MD, USA, 21218. [email protected], [email protected], [email protected], [email protected]
R. Morganti
Affiliation:
Netherlands Foundation for Astronomy, PO Box 2, Dwingeloo, Holland 7990 AA. [email protected]
C. N. Tadhunter
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore MD, USA, 21218. [email protected], [email protected], [email protected], [email protected]
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Abstract

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We have obtained long slit spectra of 3C 67 and 3C 277.1 with the HST/STIS spectrograph. We present our preliminary results on the diagnostic emission line ratios along the radio source axes in 3C 67 and 3C 277.1.

Type
GPS/CSS Workshop
Copyright
Copyright © Astronomical Society of Australia 2003

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