Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 2009
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aspc..419...96g&link_type=abstract
Galaxy Evolution: Emerging Insights and Future Challenges ASP Conference Series, Vol. 419, proceedings of a conference held 11-1
Astronomy and Astrophysics
Astronomy
Scientific paper
We demonstrate that the stellar populations of early type galaxies span a 2-D space, which means that their star formation histories form a two-parameter family. This two-parameter family maps onto a cross section through the Fundamental Plane (FP), suggesting a strong correlation between the present day structure of a galaxy and its past star formation history. The observed stellar population differences translate into M*/L variations that are too small to explain either the tilt of the FP or its thickness. This implies that the tilt and thickness of the FP are driven by systematic variations in either the central dark matter fraction in galaxies or in the IMF with which they form stars. Furthermore, because star formation histories can be mapped onto locations in FP-space, the variations in central dark matter fraction or IMF differences must be correlated with differences in the galaxies’ star formation histories.
No associations
LandOfFree
Stellar Populations and Mass-to-Light Ratios Throughout the Fundamental Plane 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 Stellar Populations and Mass-to-Light Ratios Throughout the Fundamental Plane, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Stellar Populations and Mass-to-Light Ratios Throughout the Fundamental Plane will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1112068