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Astron. Astrophys. 352, L51-L56 (1999)

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5. Conclusions

Because of its enormous Ly[FORMULA] luminosity and strong continuum, its highly asymmetric and broad Ly[FORMULA] profile, and its very asymmetric radio/near-IR morphology TN J1338-1942 is a unique laboratory for studying the nature of [FORMULA] HzRGs. It is particularly important to investigate the statistical properties of similar objects by extending the work begun here to a significant sample of [FORMULA] HzRGs. The VLT will be a crucial facility in such a study.

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© European Southern Observatory (ESO) 1999

Online publication: November 23, 1999
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