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Cited article:

Bar-driven Gas Dynamics of M31

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Large-scale Hydrodynamical Shocks as the Smoking-gun Evidence for a Bar in M31

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Evidence for non-axisymmetry in M 31 from wide-field kinematics of stars and gas

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Sculpting Andromeda – made-to-measure models for M31’s bar and composite bulge: dynamics, stellar and dark matter mass

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Monthly Notices of the Royal Astronomical Society 481 (3) 3210 (2018)
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Structure and dynamics of galaxies with a low surface-brightness disc - I. The stellar and ionized-gas kinematics

A. Pizzella, E. M. Corsini, M. Sarzi, et al.
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Unveiling the Boxy Bulge and Bar of the Andromeda Spiral Galaxy

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Sp i t zer MIPS Infrared Imaging of M31: Further Evidence for a Spiral-Ring Composite Structure

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The Astrophysical Journal 638 (2) L87 (2006)
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Investigating the Andromeda stream — I. Simple analytic bulge—disc—halo model for M31

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Substructure around M31: Evolution and Effects

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Self‐Gravitating Eccentric Disk Models for the Double Nucleus of M31

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Minor-axis velocity gradients in spirals and the case of inner polar disks$^{\bf,}$

E. M. Corsini, A. Pizzella, L. Coccato and F. Bertola
Astronomy & Astrophysics 408 (3) 873 (2003)
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ΛCDM‐based Models for the Milky Way and M31. I. Dynamical Models

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The Astrophysical Journal 573 (2) 597 (2002)
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