We discuss some recent integral field spectroscopy using the SAURON instrument of a sample consisting of 24 early-type spirals, part of the SAURON Survey, and 18 late-type spirals. Using 2-dimensional maps of their stellar radial velocity, velocity dispersion, and absorption line strength, it is now much easier to understand the nature of nearby galactic bulges. We discuss a few highlights of this work, and point out some new ideas about the formation of galactic bulges. © 2008 Copyright International Astronomical Union 2008.
CITATION STYLE
Peletier, R. F., Ganda, K., Falcón-Barroso, J., Bacon, R., Cappellari, M., Davies, R. L., … Van De Ven, G. (2007). Spiral galaxies in the SAURON survey. In Proceedings of the International Astronomical Union (Vol. 3, pp. 271–276). https://doi.org/10.1017/S1743921308017894
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