L. A. M. Tasca, O. Le Fevre, C. Lopez-Sanjuan, P. -W. Wang, P. Cassata, B. Garilli, O. Ilbert, V. Le Brun, B. C. Lemaux, D. Maccagni, L. Tresse, S. Bardelli, T. Contini, O. Cucciati, A. Fontana, M. Giavalisco, J. -P. Kneib, M. Salvato, Y. Taniguchi, D. Vergani, G. Zamorani, E. Zucca
The mass assembly of galaxies can proceed through different physical processes. Here we report on the spectroscopic identification of close physical pairs of galaxies at redshifts 2 View original: http://arxiv.org/abs/1303.4400
No comments:
Post a Comment