Photometry and long-slit spectroscopy are presented for 14 S0 and spiral galaxies of the Fornax, Eridanus and Pegasus clusters and the NGC 7582 group. The age, metallicity and \u3b1/Fe enhancement of the stellar population in the centres and their gradients are obtained using stellar population models with variable element abundance ratios. Most of the sample bulges display solar \u3b1/Fe enhancement, no gradient in age, and a negative gradient of metallicity. One of the bulges, that of NGC 1292, is a pseudobulge and the properties of its stellar population are consistent with a slow build-up within a scenario of secular evolution
A major aim of current astrophysical research is the development of models of galaxy formation that ...
We present extensive photometric and spectroscopic study to give a new insight in the bulge stellar ...
Key information to understand the formation and evolution of disk galaxies are imprinted in the stel...
Photometry and long-slit spectroscopy are presented for 14 S0 and spiral galaxies of the Fornax, Eri...
Photometry and long-slit spectroscopy are presented for 14 S0 and spiral galaxies of the Fornax, Eri...
The radial profiles of the age, metallicity and α/Fe enhancement of the stellar populations in the b...
The radial profiles of the Hβ, Mg, and Fe line-strength indices are presented for a sample of eight ...
The radial profiles of the H\u3b2, Mg, and Fe line-strength indices are presented for a sample of ei...
‘The definitive version is available at www.blackwell-synergy.com.’ Copyright Blackwell Publishing /...
We present the radial profiles of the age, metallicity and alpha/Fe enhancement of the stellar popul...
We investigated the properties of the stellar populations in the discs of a sample of 10 spiral gala...
We present the radial profiles of the Hβ, Mg and Fe line-strength indices for a sample of eight spir...
We investigated the properties of the stellar populations in the discs of a sample of 10 spiral gala...
We investigated the properties of the stellar populations in the discs of a sample of 10 spiral gala...
We investigated the properties of the stellar populations in the discs of a sample of 10 spiral gala...
A major aim of current astrophysical research is the development of models of galaxy formation that ...
We present extensive photometric and spectroscopic study to give a new insight in the bulge stellar ...
Key information to understand the formation and evolution of disk galaxies are imprinted in the stel...
Photometry and long-slit spectroscopy are presented for 14 S0 and spiral galaxies of the Fornax, Eri...
Photometry and long-slit spectroscopy are presented for 14 S0 and spiral galaxies of the Fornax, Eri...
The radial profiles of the age, metallicity and α/Fe enhancement of the stellar populations in the b...
The radial profiles of the Hβ, Mg, and Fe line-strength indices are presented for a sample of eight ...
The radial profiles of the H\u3b2, Mg, and Fe line-strength indices are presented for a sample of ei...
‘The definitive version is available at www.blackwell-synergy.com.’ Copyright Blackwell Publishing /...
We present the radial profiles of the age, metallicity and alpha/Fe enhancement of the stellar popul...
We investigated the properties of the stellar populations in the discs of a sample of 10 spiral gala...
We present the radial profiles of the Hβ, Mg and Fe line-strength indices for a sample of eight spir...
We investigated the properties of the stellar populations in the discs of a sample of 10 spiral gala...
We investigated the properties of the stellar populations in the discs of a sample of 10 spiral gala...
We investigated the properties of the stellar populations in the discs of a sample of 10 spiral gala...
A major aim of current astrophysical research is the development of models of galaxy formation that ...
We present extensive photometric and spectroscopic study to give a new insight in the bulge stellar ...
Key information to understand the formation and evolution of disk galaxies are imprinted in the stel...