Estimation of absorption line indices of early-type galaxies using colours

Details Estimation of absorption line indices of early-type galaxies using colours Estimation of absorption line indices of early-type galaxies using colours

2010-12-17

arxiv.org/abs/1012.3900v2

Astronomy and Astrophysics

Astrophysics

Galaxy Astrophysics

9 pages, 21 figures, will be shown in A&A

Scientific paper

Context. Absorption line indices are widely used to determine the stellar population parameters such as age and metallicity of galaxies, but it is not easy to obtain the line indices of some distant galaxies that have colours available. Aims. This paper investigates the correlations between absorption line indices and colours. Methods. A few statistical fitting methods are mainly used, via both the observational data of Sloan Digital Sky Survey and a widely used theoretical stellar population model. Results. Some correlations between widely used absorption line indices and ugriz colours are found from both observational data of early-type galaxies and a theoretical simple stellar population model. In particular, good correlations between colours and widely used absorption line indices such as Dn(4000), HgammaA, HgammaF, HdeltaA, Mg1, Mg2, and Mgb, are shown in this paper. Conclusions. Some important absorption line indices of early-type galaxies can be estimated from their colours using correlations between absorption line indices and colours. For example, age-sensitive absorption line indices can be estimated from (u-r) or (g-r) colours and metallicity-sensitive ones from (u - z) or (g - z). This is useful for studying the stellar populations of distant galaxies, especially for statistical investigations.

Affiliated with

Also associated with

No associations

Rating

Estimation of absorption line indices of early-type galaxies using colours does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Estimation of absorption line indices of early-type galaxies using colours, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Estimation of absorption line indices of early-type galaxies using colours will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-639193