A Principal Component Analysis approach to the Star Formation History of elliptical galaxies in Compact Groups

Details A Principal Component Analysis approach to the Star Formation History of elliptical galaxies in Compact Groups A Principal Component Analysis approach to the Star Formation History of elliptical galaxies in Compact Groups

2005-11-27

arxiv.org/abs/astro-ph/0511753v2

Mon.Not.Roy.Astron.Soc.370:828-836,2006

Astronomy and Astrophysics

Astrophysics

9 pages, 8 figures. Accepted for publication in MNRAS

Scientific paper

10.1111/j.1365-2966.2006.10509.x

(Abridged) Environmental differences in the stellar populations of early-type galaxies are explored using principal component analysis (PCA), focusing on differences between elliptical galaxies in Hickson Compact Groups (HCGs) and in the field. The method is model-independent and relies on variations between the observed spectra. The projections (PC1,PC2) reveal a difference with respect to environment, with a wider range in PC1 and PC2 in the group sample. We define a spectral parameter (zeta=0.36PC1-PC2) which simplifies this result to a single number: field galaxies have a very similar value of zeta, whereas HCG galaxies span a wide range in this parameter. We obtain a strong correlation between the values of zeta and the mass fraction in younger stars, so that some group galaxies present a higher fraction of them. PCA is more sensitive than other methods based on a direct analysis of observables such as the structure of the surface brightness profile or the equivalent width of absorption lines. The latter do not reveal any significant variation between field and compact group galaxies. Our results imply that the presence of young stars only amounts to a fraction of a percent in its contribution to the total variance.

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