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# Spectroscopy of the Double Quasars Q1343+266AB: I. a New Determination of the Size of Lyman-Alpha Forest Absorbers

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### Abstract

We have obtained spectroscopy of Q 1343+266 AB, a pair of quasars at redshift z = 2.03 with a projected separation of 9.5 arcseconds. This system is well-suited for probing the Ly-alpha forest, since the two component spectra show several Ly-alpha lines in common and several others not. Using Bayesian statistics, under the idealization of uniform-radius spherical absorbers, we find that the Ly-alpha cloud radius at $$z \approx 1.8$$ lies in the range $$40\hkpc < R < 280 \hkpc$$ with $$98\%$$ confidence in a $$(\Omega_o, \Lambda_o) = (1, 0)$$ model universe, where $$h =(H_o / 100 km s^{-1} Mpc^{-1})$$. The median value of R is 90 h^-1 kpc. \ These numbers scale up by a factor 1.44 for $$(\Omega_o, \Lambda_o) =(0.1, 0)$$; and by a factor 1.85 for (0.1, 0.9). Pressure-confined and freely-expanding Ly-alpha cloud models in which the absorbers formed in a significantly more compressed state at $$z \gg 2$$ are contradicted by these new data, as are models involving stably-confined gas concentrations in photoionization equilibrium within minihalos of cold dark matter. The comoving density of Ly-alpha forest objects at $$z\sim 2$$ is $$\sim 0.3 h (R/100 kpc)^{-2} Mpc^{-3}$$ in a (1,0) model universe. This suggests a possible identification of Ly-alpha clouds with the unvirialized, collapsing progenitors of the faint, blue galaxies at $$z\sim 1$$.

### Author and article information

###### Journal
02 September 1994
astro-ph/9409007
10.1086/187688