The pseudobulge of NGC 1292
Astrophysics
2008-02-06 v1
Abstract
The photometric and kinematic properties of Sb NGC 1292 suggest it hosts a pseudobulge. The properties of the stellar population of such a pseudobulge are consistent with a slow buildup within a scenario of secular evolution.
Keywords
Cite
@article{arxiv.0802.0610,
title = {The pseudobulge of NGC 1292},
author = {L. Morelli and E. Pompei and A. Pizzella and J. Méndez-Abreu and E. M. Corsini and L. Coccato and R. P. Saglia and M. Sarzi and F. Bertola},
journal= {arXiv preprint arXiv:0802.0610},
year = {2008}
}
Comments
2 pages, 1 figure to appear in the proceedings of "Formation and Evolution of Galaxy Disks", Rome, October 2007, Eds. J. Funes and E. M. Corsini