Plausible fluorescent Ly-alpha emitters around the z=3.1 QSO0420-388

Abstract

We report the results of a survey for fluorescent Ly-alpha emission carried out in the field surrounding the z=3.1 quasar QSO0420-388 using the FORS2 instrument on the VLT. We first review the properties expected for fluorescent Ly-alpha emitters, compared with those of other non-fluorescent Ly-alpha emitters. Our observational search detected 13 Ly-alpha sources sparsely sampling a volume of ~14000 comoving Mpc^3 around the quasar. The properties of these in terms of i) the line equivalent width, ii) the line profile and iii) the value of the surface brightness related to the distance from the quasar, all suggest that several of these may be plausibly fluorescent. Moreover, their number is in good agreement with the expectation from theoretical models. One of the best candidates for fluorescence is sufficiently far behind QSO0420-388 that it would imply that the quasar has been active for (at least) ~60 Myrs. Further studies on such objects will give information about proto-galactic clouds and on the radiative history (and beaming) of the high-redshift quasars.

10 pages, 4 figures.Update to match the version published on ApJ 657, 135, 2007 March 1

References in corpus (2)

• Where is the Molecular Hydrogen in Damped Lyman-Alpha Absorbers?
• Fluorescent Lyman-alpha Emission from Gas Near a QSO at Redshift 4.28

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