To be published in:
Proceedings of the Rome Meeting:
"THE YOUNG UNIVERSE: Galaxy Formation and Evolution at Intermediate and High Redshift",
Osservatorio Astronomico di Monteporzio Catone (Roma), Italy Sept. 29 - Oct 3, 1997
1 Institut d'Astrophysique de Paris - CNRS, 98bis Bd Arago, F-75014, Paris, France
2 Institut d'Astrophysique et de Géophysique - Université de Liège, Avenue de Cointe 5, 4000 Liège, Belgium
3 NASA-Goddard Space Flight Center, Code 681, Greenbelt, MD 20771, USA
4 Astrophysikalisches Institut Postdam, An der Sternwarte 16, D-14482 Postdam, Germany
5European Southern Observatory, Schwarzschild Strasse 2, D-80547 Garching, Germany
* Directeur de Recherches FNRS, Belgium
The spatial distribution of the Ly forest is studied using new HST data of the quasar pair Q1026-0045 A and B at zem = 1.438 and 1.520 respectively. The angular separation is 36 arcsec and corresponds to transverse linear separations between lines of sight of ~300 h50-1 kpc (q0 = 0) over the redshift range 0.833 < z < 1.438. From the observed number of coincident and anti-coincident Ly absorption lines, we conclude that, at this redshift, the Ly structures have typical dimensions of ~500 h50-1 kpc, larger than the mean separation of the two lines of sight. The velocity difference, V, between coincident lines is surprinsingly small (4 and 8 pairs with V < 50 and 200 km s-1 respectively).
There is a metal poor associated system at zabs = 1.4420 along the line of sight to A with complex velocity profile. We detect a strong Ly absorption along the line of sight to B redshifted by only 300 km s-1 relatively to the associated system. Given the strong proximity effect from quasar A, it is tempting to interpret this as the presence of a disk of radius larger than ~300 h50-1 kpc surrounding quasar A.
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