Sheets and Filaments as the Origin of the High-Velocity Tail of the Lyman-Alpha Forest
arXiv:astro-ph/9707334 · doi:10.1086/305899
Abstract
Simulations of large-scale structure formation predict the formation of sheet- and filamentary structures, which are often invoked as the origin of the Lyman-alpha forest. In their simplest description, these sheets and filaments require a differential distribution of observed line-of-sight velocity widths () which will decrease as power-laws at velocities well above the observed peak in this distribution: for filaments, the differential distribution is , while for sheets it is . These functional dependences on arise a priori due to the geometry of these absorbing structures -- assuming random orientations relative to the line-of-sight -- and are otherwise unrelated to the physical state in the absorbing structure. We find the the distribution at in three previously published data sets to be steeper than (99.99% confidence). This implies that evidence of the finite length of these kinds of absorbing structures is present in the -distribution data.
arXiv comment12 pages, 2 figures, Latex, requires aaspp4.sty,12pt.sty,flushrt.sty; Submitted, ApJ Letters
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