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The Proximity Effect on the Lyman α Forest Due to a Foreground QSO

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QSO Absorption Lines

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

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Abstract

We present the results of our study on three close pairs of QSOs. Our results are consistent with the existence of a proximity effect. due to the foreground QSO, but due to its weakness we can only reject the absence of such effect at ~ 1σ level. By modeling this proximity effect in terms of a simple photoionisation model, we find the best value for the UV ionizing background to be ~ 10−20.5 erg cm−2 s−1 Hz−1 srad−1 at the Lyman limit, and an absolute lower limit (95% confidence) of 10−21.8 erg cm−2 s−1 Hz−1 srad−1. This lower limit rejects a number of models for the UV background where it is mostly contributed by QSOs and absorption by Lyman limit systems is taken into account.

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© 1995 Springer-Verlag Berlin Heidelberg

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Fernández-Soto, A., Barcons, X., Carballo, R., Webb, J.K. (1995). The Proximity Effect on the Lyman α Forest Due to a Foreground QSO. In: Meylan, G. (eds) QSO Absorption Lines. ESO Astrophysics Symposia. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-540-49458-4_60

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  • DOI: https://doi.org/10.1007/978-3-540-49458-4_60

  • 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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