Masao Mori, Astrophysics, University of Tsukuba
Theoretical Astrophysics and Computational Physics

Andromeda streams · 2008 · Journal article

What does M31’s surviving disc tell us about the satellite that formed its giant stream?

A live N-body model follows both tidal debris and the response of Andromeda to an accreted satellite.

The Once and Future Andromeda Stream

The Once and Future Andromeda Stream. Mori, Masao; Rich, R. Michael, Astrophysical Journal, 674, L77 (2008).

Approach

A forty-million-particle simulation includes self-gravitating disc, bulge and halo components and follows the encounter several billion years forward.

Main result

The stream and eastern and western shells are reproduced. Preserving the observed disc limits the satellite mass to about five billion solar masses in the model.

Scientific implications

Disc survival complements debris morphology as a constraint on the strength of a past merger.

Scope and limitations

The mass bound depends on the assumed encounter and M31 structure. Proposed links to older diffuse arcs are dynamical interpretations, not uniquely established histories.

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