Morphological number counts and redshift distributions to I &lt;26 from the Hubble deep field: Implications for the evolution of ellipticals, spirals, and irregulars

Morphological number counts and redshift distributions to I <26 from the Hubble deep field: Implications for the evolution of ellipticals, spirals, and irregulars

Journal article published in 1998 by Driver Sp, A. Fernandez Soto, Couch Wj, Odewahn Sc, Windhorst Ra, Steven Phillipps

, K. Lanzetta, A. Yahil

This paper was not found in any repository; the policy of its publisher is unknown or unclear.

Full text: Unavailable

Preprint: policy unknown

Upload

Postprint: policy unknown

Upload

Published version: policy unknown

Upload