Investigating the Andromeda stream — I. Simple analytic bulge—disc—halo model for M31
Open Access
- 1 March 2006
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 366 (3) , 996-1011
- https://doi.org/10.1111/j.1365-2966.2005.09863.x
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This publication has 66 references indexed in Scilit:
- Improving the triaxial bulge model of M31Monthly Notices of the Royal Astronomical Society, 2002
- A New Formation Model for M32: A Threshed Early-Type Spiral Galaxy?The Astrophysical Journal, 2001
- The M 31 double nucleus probed with OASIS and HSTAstronomy & Astrophysics, 2001
- Hydrodynamic simulations of the triaxial bulge of M 31Astronomy & Astrophysics, 2001
- Stellar Mass‐to‐Light Ratios and the Tully‐Fisher RelationThe Astrophysical Journal, 2001
- Profiles of dark haloes: evolution, scatter and environmentMonthly Notices of the Royal Astronomical Society, 2001
- M31 Globular Clusters: Colors and MetallicitiesThe Astronomical Journal, 2000
- The distribution and kinematics of neutral gas in M31The Astrophysical Journal, 1991
- Contraction of dark matter galactic halos due to baryonic infallThe Astrophysical Journal, 1986
- Spectrographic Observations of the Rotation of the Andromeda NebulaPublications of the Astronomical Society of the Pacific, 1938