1998A&A...334L..45P

The spatial distribution of the Lyα forest is studied using new HST data for the quasar pair Q 1026-0045 A and B at z_em=1.438 and 1.520 respectively. The angular separation is 36 arcsec and corresponds to transverse linear separations between lines of sight of ∼300h^–1₅₀kpc (q₀=0.5) over the redshift range 0.833<z<1.438. From the observed numbers of coincident and anti-coincident Lyα absorption lines, we conclude that, at this redshift, the Lyα structures have typical dimensions of ∼500h^–1₅₀kpc, larger than the mean separation of the two lines of sight. The velocity difference, {DELTA}V, between coincident lines is surprisingly small (4 and 8 pairs with {DELTA}V<50 and 200km/s respectively). Metal line systems are present at z_abs=1.2651 and 1.2969 in A, z_abs=0.6320, 0.7090, 1.2651 and 1.4844 in B. In addition we tentatively identify a weak Mg II system at z_abs=0.11 in B. It is remarkable that the z_abs=1.2651 system is common to both lines of sight. The system at z_abs=1.4844 has strong O vi absorption. There is a metal-poor associated system at z_abs=1.4420 along the line of sight to A with complex velocity profile. We detect a strong Lyα absorption along the line of sight to B redshifted by only 300km/s relatively to the associated system. It is tempting to interpret this as the presence of a disk of radius larger than 300h^–1₅₀kpc surrounding quasar A.