Induced star formation and morphological evolution in very high redshift radio galaxies

Near-infrared, sub-arcsecond seeing images obtained with the W M Keck I Telescope of show strong evolution at rest-frame optical wavelengths in the morphologies of high redshift radio galaxies (HzRGs) with 1 9 3, to much more compact and symmetrical shapes at z 3 HzRGs are similar to the total sizes and luminosities of normal, radio-quiet, star forming galaxies seen at z = 3 - 4 `R`-band, 0 1`` resolution images with the Hubble Space Telescope of one of these HzRGs, 4C41 17 at z = 3 800, show that at rest-frame UV wavelengths the galaxy morphology breaks up in even smaller, {approximately} 1 kpc-sized components embedded in a large halo of low suface brightness emission The brightest UV emission is from a radio-aligned, edge-brightened feature (4C41 17.North) downstream from a bright radio knot A narrow-band Ly-{alpha} image, also obtained with HST, shows an arc-shaped Ly-{alpha} feature at this same location, suggestive of a strong jet/cloud collision Deep spectropolarimetric observations with the W M Keck II Telescope of 4C41 17 show that the radio-aligned UV continuum is unpolarized Instead the total light spectrum shows ahsorption lines and P-Cygni type features that are similar to the radio-quiet z = 3 - 4 star forming galaxies This shows that the rest-frame UV light in 4C41 17 is dominated by starlight, not scattered light from a hidden AGN The combined HST and Keck data suggest that the radio--aligned rest-frame UV continuum is probably caused by jet-induced star formation The strong morphological evolution suggests that we see the first evidence for the assemblage of massive ellipticals, the parent population of very powerful radio sources at much lower redshifts The presence of radio aligned features in many of the z > 3 HzRGs suggests, by analogy to 4C41 17, that jet-induced star formation may be a common phenomenon in these galaxies in their early stages of formation