Abstract
We present first results of a comprehensive survey of deep long-slit spectra along the minor axis of bulges of edge-on spiral galaxies. Our results indicate that stellar populations in bulges are fairly old and encompass a range of metallicities. The luminosity-weighted ages of bulges range from those found for cluster ellipticals to slightly `younger' (by up to only a few Gyr, however). Their α/Fe element ratio is typically supersolar, consistent with those found in giant ellipticals. The radial line-strength gradients in bulges correlate with bulge luminosity. Generally, these findings are more compatible with predictions of the `dissipative collapse' model than with those of the `secular evolution' model.
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Goudfrooij, P., Gorgas, J. & Jablonka, P. Line Strengths and Line Strength Gradients in Bulges along the Hubble Sequence. Astrophysics and Space Science 269, 109–116 (1999). https://doi.org/10.1023/A:1017015808447
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DOI: https://doi.org/10.1023/A:1017015808447