Formation of the Small Magellanic Cloud: ancient major merger as a solution to the kinematical differences between old stars and HI gas

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Bekki, Kenji; Chiba, Masashi;
  • Identifiers: doi: 10.1086/589441
  • Subject: Astrophysics
    arxiv: Astrophysics::Galaxy Astrophysics | Astrophysics::Cosmology and Extragalactic Astrophysics | Astrophysics::Earth and Planetary Astrophysics | Astrophysics::Solar and Stellar Astrophysics

Recent observations of the Small Magellanic Cloud (SMC) have revealed that the HI gas shows a significant amount of rotation (V_c 60 km/s), while no or little rotation is evident for the old stellar populations. We suggest that this unique kinematical difference between... View more
  • References (2)

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    Demers, S., Battinelli, P., & Artigau, E. 2006, A&A, 456, 905 Cioni, M.-R. L., Habing, H. J., & Israel, F. P. 2000, A&A, 358, L9

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