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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. labiano@stsci.edu, odea@stsci.edu, sbaum@stsci.edu, koekemoe@stsci.edu Kapteyn Astronomical Institute, PO Box 800, Groningen, Holland, 9700 AV. pdb@astro.rug.nl, labiano@astro.rug.nl
C. P. O'Dea
Affiliation:
Western Kentucky University, 1 Big Red Way, Bowling Green KY, USA 42101-3576. gelderman@wku.edu
R. Gelderman
Affiliation:
Lawrence Livermore National Laboratory, 7000 East Avenue, Livermore CA, USA 94550-9234. wdevries@igpp.ucllnl.org
W. H. de Vries
Affiliation:
University of Hertfordshire, College Lane, Hatfield Herts, UK AL10 9AB. dja@star.herts.ac.uk
D. J. Axon
Affiliation:
University of Hertfordshire, College Lane, Hatfield Herts, UK AL10 9AB. dja@star.herts.ac.uk
P. D. Barthel
Affiliation:
Kapteyn Astronomical Institute, PO Box 800, Groningen, Holland, 9700 AV. pdb@astro.rug.nl, labiano@astro.rug.nl
S. A. Baum
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore MD, USA, 21218. labiano@stsci.edu, odea@stsci.edu, sbaum@stsci.edu, koekemoe@stsci.edu
A. Capetti
Affiliation:
Osservatorio Astronomico di Torino, Via Osservatorio 20, Pino Torinesse (TO), Italy 10025. capetti@to.astro.it
R. Fanti
Affiliation:
Instituto di Radioastronomia del CNR, Via P. Gobetti, 101, Bologna, Italy 40129. rfanti@ira.bo.cnr.it
A. M. Koekemoer
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore MD, USA, 21218. labiano@stsci.edu, odea@stsci.edu, sbaum@stsci.edu, koekemoe@stsci.edu
R. Morganti
Affiliation:
Netherlands Foundation for Astronomy, PO Box 2, Dwingeloo, Holland 7990 AA. morganti@nfra.nl
C. N. Tadhunter
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore MD, USA, 21218. labiano@stsci.edu, odea@stsci.edu, sbaum@stsci.edu, koekemoe@stsci.edu
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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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