The Structure of High Redshift Galactic Halos

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dc.creatorEllison, Sara L.
dc.creatorIbata, Rodrigo
dc.creatorPettini, Max
dc.creatorLewis, Geraint F.
dc.creatorAracil, Bastien
dc.creatorPetitjean, Patrick
dc.creatorSrianand, R.
dc.date2003-09-11
dc.date.accessioned2026-07-07T02:09:31Z
dc.date.available2026-07-07T02:09:31Z
dc.descriptionObservations of multiple or lensed QSOs at high redshift can be used to probe transverse structure in intervening absorption systems. Here we present results obtained from STIS spectroscopy of the unique triply imaged QSO APM08279+5255 at z = 3.9 and study the coherence scales of intervening low and high ionization absorbers.
dc.descriptionTo appear in `Recycling Intergalactic and Interstellar Matter', IAU Symposium series, vol 217, Eds P.-A. Duc, J. Braine, E. Brinks
dc.identifierhttps://arxiv.org/abs/astro-ph/0309308
dc.identifierhttp://arxiv.org/abs/astro-ph/0309308
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/6459
dc.subjectAstrophysics
dc.titleThe Structure of High Redshift Galactic Halos
dc.typetext

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