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

  • A. Labiano (a1) (a2), C. P. O'Dea (a3), R. Gelderman (a4), W. H. de Vries (a5), D. J. Axon (a5), P. D. Barthel (a2), S. A. Baum (a1), A. Capetti (a6), R. Fanti (a7), A. M. Koekemoer (a1), R. Morganti (a8) and C. N. Tadhunter (a1)...

Abstract

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.

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References

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Baldwin, J. A., Philips, M. M., & Terlevich, T. PASP, 1981, 93, 5
Cardelli, J. A., Clayton, C., & Mathis, J. S. ApJ, 1989, 345, 245
de Vries, W. H., O'Dea, C. P., Baum, S. A., & Barthel, P. D. 1999, ApJ, 526, 27
de Vries, W. H., et al. 1997, ApJS, 110, 191
Ferland, G. J., & Netzer, H. ApJ, 1983, 264, 105
Freedman, W. L., et al. 2001, ApJ, 553, 47
Gelderman, R., & Whittle, M. 1994, ApJS, 91, 491
Heckman, T. M. 1980, A&A, 87, 152
Kriss, G. 1994, PASP, 61, 437
Moy, E., & Rocca-Volmerange, B. 2002, A&A, 383, 46
O'Dea, C. P., et al. 2002, AJ, 123, 2333
Schlegel, J. D., Finkbeiner, D. P., & Davis, M. ApJ, 1998, 500, 525

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