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

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 $h=(H_o/100km{s}^{-1}Mp{c}^{-1})$. 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 $\sim 0.3h(R/100kpc{)}^{-2}Mp{c}^{-3}$ 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 $z\sim 1$.

(9 pages, Accepted to Ap. J. Letters) 9294