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| Paper: |
The Impact of Stellar Populations on the Dynamics of Merger Remnants |
| Volume: |
423, Galaxy Wars: Star Formation and Stellar Populations in Interacting Galaxies |
| Page: |
351 |
| Authors: |
Rothberg, B.; Fischer, J. |
| Abstract: |
Many studies and simulations suggest gas-rich mergers do not contribute significantly to the overall star-formation rate and total mass function of galaxies. The velocity dispersions (σ) of Luminous & Ultraluminous Infrared Galaxies measured using the 1.62 or 2.29 μm CO bandheads imply they will form m < m* ellipticals. Yet, σ’s obtained with the Calcium II triplet (CaT) at 0.85μm suggest all types of mergers will form m > m* ellipticals. Presented here are recent results, based on high-resolution imaging and multi-wavelength spectroscopy, which demonstrate the dominance of a nuclear disk of Red Supergiants (RSG) or Asymptotic Giant Branch (AGB) stars in the near-infrared bands, where dust obscuration does not sufficiently block their signatures. The presence of these stars severely biases the dynamical mass. At I-band, where dust can sufficiently block RSG or AGB stars, LIRGs populate the Fundamental Plane over a large dynamic range and are virtually indistinguishable from elliptical galaxies. |
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