The very late-stage merger IC 4200:pre-elliptical or pre-spiral?
Astrophysics
2007-05-23 v1
Abstract
Recent observations have revealed a class of unusually HI-rich early-type galaxies. By combining observations of their morphology, stellar populations and neutral hydrogen we aim to understand how these galaxies fit into the hierarchical formation paradigm. Here we present the result of our radio and optical observations of a test case galaxy, the E/S0 IC 4200.
Cite
@article{arxiv.astro-ph/0509350,
title = {The very late-stage merger IC 4200:pre-elliptical or pre-spiral?},
author = {P. Serra and S. C. Trager and J. M. van der Hulst and T. A. Oosterloo and R. Morganti and J. H. van Gorkom},
journal= {arXiv preprint arXiv:astro-ph/0509350},
year = {2007}
}
Comments
Proceedings for the 5th Marseille International Cosmology Conference: The Fabulous Destiny of Galaxies. (2 pages)