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High resolution spectroscopy of absorption lines in the Z = 1.7 BL Lac object 0215+015*

Published online by Cambridge University Press:  19 July 2016

J. Chris Blades ,
Richard W. Hunstead ,
Hugh S. Murdoch  and
Max. Pettini
J. Chris Blades
Affiliation:
Space Telescope Science Institute Richard W. Hunstead
Richard W. Hunstead
Affiliation:
School of Physics, University of Sydney
Hugh S. Murdoch
Affiliation:
School of Physics, University of Sydney
Max. Pettini
Affiliation:
Royal Greenwich Observatory

Extract

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We describe the various absorption systems in 0215+015, and present results from our new, high-resolution studies at 10 km/sec (FWHM).

Type
VI. Quasars as Probes of the Intervening Medium
Information
Symposium - International Astronomical Union , Volume 119: Quasars , 1986 , pp. 571 - 572
Copyright
Copyright © Reidel 1986 

References

Bergeron, J. and d'Odorico, S., 1985, preprint.Google Scholar
Blades, J. C., Hunstead, R. W., Murdoch, H. S. and Pettini, M., 1985, Ap. J., 288, 580.Google Scholar
Gaskell, C. M., 1982, Ap. J., 252, 447.CrossRefGoogle Scholar
Hartquist, T., Pettini, M. and Tallant, A., 1984, Ap. J., 276, 519.Google Scholar
Pettini, M., 1985, ESO Workshop on Production and Distribution of C, N, O Elements, Munich.Google Scholar
Pettini, M., Hunstead, R. W., Murdoch, H. S. and Blades, J. C., 1983, Ap. J., 273, 436.CrossRefGoogle Scholar
York, D. G., 1982, Ann. Rev. Ast. Astrophys., 20, 221.CrossRefGoogle Scholar