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Investigation into the Origin of Age-Velocity dispersion Relation by High Resolution Simulation

  • Jun Kumamoto (a1) (a2), Junichi Baba (a2) and Takayuki R. Saitoh (a2)

Abstract

We focused on the stellar age-velocity dispersion relation (AVR). We performed the N-body/SPH simulations to investigate the origin of AVR. As a results, we found that AVR is not consistent with simple stellar heating.

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References

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Hänninen, J. & Flynn, C. 2002, MNRAS, 337, 731
Holmberg, J., Nordström, B., & Andersen, J. 2009, A&A, 501, 941
Saitoh, T. R., Daisaka, H., Kokubo, E., Makino, J., Okamoto, T., Tomisaka, K., Wada, K., & Yoshida, N. 2008, PASJ, 60, 667
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Keywords

Investigation into the Origin of Age-Velocity dispersion Relation by High Resolution Simulation

  • Jun Kumamoto (a1) (a2), Junichi Baba (a2) and Takayuki R. Saitoh (a2)

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