Ly-alpha absorbers at z<1 : HST-CFHT imaging and spectroscopy in the field of 3C 286

dc.creatorBrun, V. Le
dc.creatorBergeron, J.
dc.date1998-01-29
dc.date.accessioned2026-07-25T20:42:50Z
dc.descriptionWe present further observational results on our Lya-only absorber identification project at low and intermediate redshifts. We combine CFHT/MOS imaging and spectroscopic observations of 25 galaxies in the field of the quasar 3C286 (z_e = 0.849) with HST/FOS spectrum of the quasar between 1600 and 3000 A and HST/WFPC2 high spatial resolution imaging of some galaxies. Our results confirm our first conclusions on the nature of the intermediate redshift Ly-alpha forest absorbers. A small fraction of them is tightly linked to galaxies, and most probably arise in the external parts of giant halos (R~200 kpc with H0=50 km/s/Mpc) around fairly luminous galaxies (M_AB(B) < -19) of various spectral and morphological types, as shown by HST imaging of these objects. Most of the absorbing clouds appear to be only ``associated'' with galaxies, in the sense that they could trace the gaseous filaments or sheets of large-scale structures. Thus, as expected from a sample tracing large scale structures, these galaxies have various spectral types. We also find that groups of galaxies have always at least one associated Ly-alpha absorption line.
dc.descriptionaccepted for publication in A&A main journal. 12 pages, 16 figures, uses aa.cls
dc.identifierhttps://arxiv.org/abs/astro-ph/9801302
dc.identifierhttp://arxiv.org/abs/astro-ph/9801302
dc.identifier.urihttps://dspace.dare.co.zw/handle/123456789/72457
dc.subjectAstrophysics
dc.titleLy-alpha absorbers at z<1 : HST-CFHT imaging and spectroscopy in the field of 3C 286
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