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Patchy intergalactic HeII absorption in HE 2347-4342. - The possible discovery of the epoch of He-reionization | | D. Reimers
; S. Koehler
; L. Wisotzki
; D. Groote
; P. Rodriguez-Pascual
; W. Wamsteker
; | | Date: |
15 Jul 1997 | | Subject: | astro-ph | | Abstract: | We report on observations of redshifted HeII 304 A absorption in the QSO HE 2347-4342 (z=2.885, V=16.1) with the GHRS on board HST (FWHM=0.7 A). At the expected position of HeII 304 A absorption, HE 2347-4342 is the most UV-bright high redshift QSO discovered so far. We show that the HeII opacity as a function of redshift is patchy showing spectral regions with low HeII opacity (voids) and regions with high HeII opacity (troughs) and no detectable flux. Combination with high-resolution optical spectra of the Ly_alpha forest using CASPEC at the ESO 3.6m telescope shows that the voids can be explained either exclusively by Ly_alpha forest cloud absorption with a moderate N(HeII)/N(HI) ratio of 100 and turbulent line broadening or by a combination of Ly_alpha forest with N(HeII)/N(HI)=45 and thermal broadening plus a diffuse medium with tau_GP_HeII=0.3. Thus a strict upper limit to a diffuse medium is Omega_diff<= 0.02 h_50^(-1.5) at z=2.8. In the troughs an additional continuous HeII 304 A opacity tau > 2.8 is required. In case of photoionization, the troughs would require a diffuse component with a density close to Omega = 0.059 h_50^(-1.5), i.e. all baryons in the universe, which is inconsistent with the observed absence of such a component in the voids. A tentative interpretation is that we observe the epoch of partial HeII reionization of the universe with patches not yet reionized. In that case a diffuse component with Omega_diff >= 1.3 10^(-4) h_50^(-1) would be sufficient to explain the ``trough’’ opacity. | | Source: | arXiv, astro-ph/9707173 | | Services: | Forum | Review | PDF | Favorites | |
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