Abstract
We present radial velocities for a sample of 723 planetary nebulae in the disc and bulge of M31, measured using the WYFFOS fibre spectrograph on the William Herschel Telescope. Velocities are determined using the [OIII] lambda 5007 emission line. Rotation and velocity dispersion are measured to a radius of 50 arcmin (11.5 kpc), the first stellar rotation curve and velocity dispersion profile for M31 to such a radius. Our kinematics are consistent with rotational support at radii well beyond the bulge effective radius of 1.4 kpc, although our data beyond a radius of 5 kpc are limited. We present tentative evidence for kinematic substructure in the bulge of M31 to be studied fully in a later work. This paper is part of an ongoing project to constrain the total mass, mass distribution and velocity anisotropy of the disc, bulge and halo of M31.
Original language | English |
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Pages (from-to) | 97-119 |
Number of pages | 23 |
Journal | Monthly Notices of the Royal Astronomical Society |
Volume | 369 |
Issue number | 1 |
DOIs | |
Publication status | Published - 11-Jun-2006 |
Keywords
- galaxies : haloes
- galaxies : individual
- M31
- galaxies : spiral
- GLOBULAR-CLUSTER SYSTEM
- SUPERMASSIVE BLACK-HOLE
- ANDROMEDA GALAXY
- RADIAL-VELOCITIES
- MICROLENSING CANDIDATES
- STELLAR-SYSTEMS
- GIANT STREAM
- KINEMATICS
- MASS
- HALO