Galaxy Interactions and Starbursts at High Redshift

(2) University of California; (3) Case Western Reserve University); A. Dekel (1); G. Rosenfeld (1); J.C. Mihos(3); Jerusalem; J.R. Primack (2) ((1) Hebrew University; R.S. Somerville (1); Santa Cruz; T.S. Kolatt (2)

arxiv: astro-ph/9910346 · v1 · submitted 1999-10-19 · 🌌 astro-ph

Galaxy Interactions and Starbursts at High Redshift

R.S. Somerville (1) , G. Rosenfeld (1) , T.S. Kolatt (2) , A. Dekel (1) , J.C. Mihos(3) , J.R. Primack (2) ((1) Hebrew University , Jerusalem , (2) University of California

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Santa Cruz (3) Case Western Reserve University)

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keywords galaxieshighinteractionsstarburstsappearanceapplybandscolor

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Using high resolution N-body simulations with hydrodynamics and star formation, we investigate interactions and the resulting starbursts in galaxies with properties typical of $z\sim 3$. We apply spectral population models to produce mock-HST images, and discuss the observed magnitude, color, and morphological appearance of our simulated galaxies in both the rest-UV and rest-visual bands.

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Galaxy Interactions and Starbursts at High Redshift

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