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The outer disk stellar populations in M31

  • R. A. Johnson (a1), D. Faria (a2), A. M. N. Ferguson (a3) and J. C. Richardson (a3)

Abstract

The outer regions of M31 contain significant substructure. Here we investigate the origins of the substructure in three fields close to the major axis of M31 using colour-magnitude diagrams produced from HST-ACS.

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References

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Faria, D., Johnson, R.A., Ferguson, A.M.N., Irwin, M.J., Ibata, R.A., Johnston, K.V., Lewis, G.F., & Tanvir, N.R. 2007, AJ accepted
Ferguson, A.M.N., Irwin, M.J., Ibata, R.A., Lewis, G.F., & Tanvir, N.R. 2002, AJ 124, 1452
Ferguson, A.M.N., Johnson, R.A., Faria, D.C., Irwin, M.J., Ibata, R.A., Johnston, K.V., Lewis, G.F., & Tanvir, N.R. 2005, ApJL 622, 109
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The outer disk stellar populations in M31

  • R. A. Johnson (a1), D. Faria (a2), A. M. N. Ferguson (a3) and J. C. Richardson (a3)

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