Abstract
We have analyzed high resolution (b ≈ 15 km/s) optical spectra of the QSO HS1700+6416 (z em = 2.72). The high S/N ratio in the Lyα forest allows a reasonable determination of the neutral hydrogen column density as well as of the velocity dispersion of the clouds. A weak, but significant, trend for stronger lines to be broader suggests that their column densities (N HI) and Doppler parameters (b) are related. A simplified model of very flattened, highly ionized clouds, gravitationally confined by dark matter, gives a good representation of the data, where the observed N HI−b correlation is due to orientation effects.
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© 1995 Springer-Verlag Berlin Heidelberg
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Rodríguez-Pascual, P.M. et al. (1995). The Lyα Forest towards HS1700+6416 at High Resolution. In: Meylan, G. (eds) QSO Absorption Lines. ESO Astrophysics Symposia. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-540-49458-4_66
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DOI: https://doi.org/10.1007/978-3-540-49458-4_66
Publisher Name: Springer, Berlin, Heidelberg
Print ISBN: 978-3-662-22373-4
Online ISBN: 978-3-540-49458-4
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