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.
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
References
Bajtlik, S., Duncan, R.C., Ostriker, J.P. (1988): ApJ, 327, 570
Bechtold, J., Weymann, R.J., Lin, Z., Malkon, M.A. (1987): ApJ, 315, 180
Fernandez-Soto, A., Barcons, X., Carballo, R., Webb, J.K. (1994): MNRAS, submitted
Madau, P. (1992): ApJ, 389, Ll
Meiksin, A. and Madau, P. (1993): ApJ, 412, 34
Author information
Authors and Affiliations
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 1995 Springer-Verlag Berlin Heidelberg
About this paper
Cite this paper
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
Download citation
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