Radiative Feedback and the Photoevaporation of Intergalactic Clouds

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dc.creatorShapiro, Paul R.
dc.creatorRaga, Alejandro C.
dc.creatorMellema, Garrelt
dc.date1998-04-12
dc.date.accessioned2026-07-25T13:11:18Z
dc.descriptionThe first sources of ionizing radiation to condense out of the dark and neutral IGM sent ionization fronts sweeping outward through their surroundings, overtaking other primordial gas-clouds and photoevaporating them. Results are presented of the first gas dynamical simulations of this process, including radiative transfer, along with some observational diagnostics.
dc.description7 pages, 6 figures. One LaTeX file, one LaTeX style file, 6 postscript files, tar-ed and gzip-ed. To appear in Proceedings of the Workshop on H_2 in the Early Universe, eds. F. Palla, E. Corbelli, and D. Galli, Memorie Della Societa Astronomica Italiana, in press (1998)
dc.identifierhttps://arxiv.org/abs/astro-ph/9804117
dc.identifierhttp://arxiv.org/abs/astro-ph/9804117
dc.identifier.urihttps://dspace.dare.co.zw/handle/123456789/15158
dc.subjectAstrophysics
dc.titleRadiative Feedback and the Photoevaporation of Intergalactic Clouds
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