Abstract
We present results on the stellar populations of a sample of 18 late-type spirals, based on data acquired with the integral-field spectrograph SAURON at the WHT. We present the two-dimensional line-strength maps, the central line indices, and estimate the star formation time-scale. In an exponentially declining SFR scenario, we find a trend between the time-scale and the central velocity dispersion: more massive galaxies show shorter burst durations. A detailed study on these data is published by Ganda et al. (2007).
Original language | English |
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Pages (from-to) | 301-302 |
Number of pages | 2 |
Journal | Proceedings of the International Astronomical Union |
Volume | 3 |
Issue number | S245 |
DOIs | |
Publication status | Published - Jul 2007 |
Externally published | Yes |
Keywords
- Galaxies: evolution
- Galaxies: individual (NGC2964)
- Galaxies: spiral