Ly-alpha excess in high redshift radio galaxies: a signature of star formation

Details Ly-alpha excess in high redshift radio galaxies: a signature of star formation Ly-alpha excess in high redshift radio galaxies: a signature of star formation

2006-12-05

arxiv.org/abs/astro-ph/0612116v1

Mon.Not.Roy.Astron.Soc.375:1299-1310,2007

Astronomy and Astrophysics

Astrophysics

14 pages, 5 figures, accepted for publication in MNRAS

Scientific paper

10.1111/j.1365-2966.2006.11371.x

About 54% of radio galaxies at z>3 and 8% of radio galaxies at 22) radio galaxies. These Ly-alpha excess objects (LAEs) show Ly-alpha/HeII values consistent with or above standard photoionization model predictions. We show that the most successful explanation is the presence of a young stellar population which provides the extra supply of ionizing photons required to explain the Ly-alpha excess in at least the most extreme LAEs (probably in all of them). The measurement of unusually high Ly-alpha ratios in the extended gas of some high redshift radio galaxies suggests that star formation activity occurs in spatial scales of tens of kpc. We argue that, although the fraction of LAEs may be incompletely determined, both at 23, the much larger fraction of LAEs found at z>3 is a genuine redshift evolution and not due to selection effects. Therefore, our results suggest that the radio galaxy phenomenon is more often associated with a massive starburst at z>3 than at z<3.

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