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Metal Line Absorptions Toward the QSO HS1700+6416

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QSO Absorption Lines

Part of the book series: ESO Astrophysics Symposia ((ESO))

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Abstract

We have analyzed high resolution (b ≈ 15 km/s) and low resolution (R ≈ 3Å) optical spectra of the QSO HS1700+6416 (z em = 2.72) taken with the ISIS spectrograph at the WHT. We are able to identify more than 50 metal lines.

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References

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Author information

Authors and Affiliations

  1. Depto. de Fisica Moderna, Univ. de Cantabria, 39005, Santander, Spain

    J. L. Sanz

  2. ESA IUE Observatory, P.O. Box 50727, 28080, Madrid, Spain

    P. M. Rodríguez-Pascual, M. C. Recondo & W. Wamsteker

  3. INSA/VILSPA, P.O. Box 50727, 28080, Madrid, Spain

    A. de la Fuente

  4. ESA ISO Observatory, P.O. Box 50727, 28080, Madrid, Spain

    J. Clavel

  5. Observatoire de Paris, RA 173 CNRS, 92135, Meudon, France

    M. Santos-Lleó

Authors
  1. J. L. Sanz
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  2. P. M. Rodríguez-Pascual
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  3. A. de la Fuente
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  4. M. C. Recondo
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  5. J. Clavel
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  6. M. Santos-Lleó
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  7. W. Wamsteker
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Editor information

Editors and Affiliations

  1. European Southern Observatory, Karl-Schwarzschild-Strasse 2, D-85748, Garching, Germany

    Georges Meylan

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© 1995 Springer-Verlag Berlin Heidelberg

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Sanz, J.L. et al. (1995). Metal Line Absorptions Toward the QSO HS1700+6416. In: Meylan, G. (eds) QSO Absorption Lines. ESO Astrophysics Symposia. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-540-49458-4_37

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  • DOI: https://doi.org/10.1007/978-3-540-49458-4_37

  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-662-22373-4

  • Online ISBN: 978-3-540-49458-4

  • eBook Packages: Springer Book Archive

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