IMAGES IV* : strong evolution of the oxygen abundance in gaseous phases of intermediate mass galaxies from z ∼ 0.8
/ Authors
M. Rodrigues, F. Hammer, H.Flores, M. Puech, Y. Liang, I. Fuentes-Carrera, N. Nesvadba, M. Lehnert, Y. Yang, P. Amram
and 42 more authors
C. Balkowski, C. Cesarsky, H.Dannerbauer, R. Delgado, B. Guiderdoni, A. Kembhavi, B. Neichel, G. Ostlin, L. Pozzetti, C. D. Ravikumar, A. Rawat, S. D. Alighieri, D. Vergani, J. Vernet, H. Wozniak, Gepi, O. Paris, Centra, I. Técnico, Lisboa, Eső, G. B. Munchen, National Astronomical Observatories, Chinese Academy of Sciences, L. D. Marseille, Mpia, Heidelberg, IFARHU-SENACYT, Panama, C. Lyon, Inter-University Centre for Astronomy, Astrophysics, Pune, Stockholm Observatory, Stockholm, I. Bologna, D. Physics, U. Calicut, -INAF, O. Arcetri, IASF-INAF, Milano
/ Abstract
Context: Intermediate mass galaxies (> 1010 M_ȯ) at z ~ 0.6 are the likeliest progenitors of the present-day, numerous population of spirals. There is growing evidence that they have evolved rap ...
Journal: Astronomy and Astrophysics