Dynamics of the Galactic Bulge using Planetary Nebulae
arXiv:astro-ph/0005086 · doi:10.1086/301504
Abstract
Evidence for a bar at the center of the Milky Way triggered a renewed enthusiasm for dynamical modelling of the Galactic bar-bulge. Our goal is to compare the kinematics of a sample of tracers, planetary nebulae, widely distributed over the bulge with the corresponding kinematics for a range of models of the inner Galaxy. Three of these models are N-body barred systems arising from the instabilities of a stellar disk (Sellwood, Fux and Kalnajs), and one is a Schwarzschild system constructed to represent the 3D distribution of the COBE/DIRBE near-IR light and then evolved as an N-body system for a few dynamical times (Zhao). For the comparison of our data with the models, we use a new technique developed by Saha (1998). The procedure finds the parameters of each model, i.e. the solar galactocentric distance R_o in model units, the orientation angle phi, the velocity scale (in km/s per model unit), and the solar tangential velocity which best fit the data.
48 pages (Latex), 30 figures (PS), accepted for pub. in AJ
References in corpus (5)
Cited by in corpus (30)
- The Galaxy in Context: Structural, Kinematic and Integrated Properties
- Our Milky Way as a Pure-Disk Galaxy -- A Challenge for Galaxy Formation
- The VST Photometric Halpha Survey of the Southern Galactic Plane and Bulge (VPHAS+)
- The Bulge Radial Velocity Assay (BRAVA): II. Complete Sample and Data Release
- Chemodynamical history of the Galactic Bulge
- Made-to-Measure models of the Galactic Box/Peanut bulge: stellar and total mass in the bulge region
- Stellar Proper Motions in the Galactic Bulge from deep HST ACS/WFC Photometry
- The Bulge Radial Velocity Assay (BRAVA): I. Techniques and a Rotation Curve
- The Bulge Radial Velocity Assay (BRAVA): I. Sample Selection and a Rotation Curve
- Models for the Gravitational Field of the Galactic Bar. An Application to Stellar Orbits in the Galactic Plane and Orbits of Some Globular Clusters
- The Pattern Speed of the OH/IR Stars in the Milky Way
- The Vertical X-shaped Structure in the Milky Way: Evidence from a Simple Boxy Bulge Model
- Planetary nebulae in the direction of the Galactic bulge: On nebulae with emission-line central stars
- Metallicity and kinematics of the bar in-situ
- Proper Motions in the Galactic Bulge: Plaut's Window
- Correlations between kinematics and metallicity in the Galactic bulge: a review
- New Planetary Nebulae in the Galactic Bulge region with l>0deg - I. Discovery method and first results
- Chemical Study of the Metal-rich Globular Cluster NGC 5927
- The vertical Na-O relation in the bulge globular cluster NGC 6553
- New Planetary Nebulae in the Galactic Bulge region with l>0deg - II
- SiO Masers in the Galactic Bulge and Disk: Kinematics from the BAaDE Survey
- Orbits of globular clusters computed with dynamical friction in the Galactic anisotropic velocity dispersion field
- The Galactic Bulge: A Review
- New groups of planetary nebulae with peculiar dust chemistry towards the Galactic bulge
- Bayesian isochrone fitting and stellar ages
- The populations of planetary nebulae in the direction of the Galactic bulge
- A new look at the kinematics of the bulge from an N-body model
- Kinematics and Composition of the Galactic Bulge: Recent Progress
- The outer halos of elliptical galaxies
- Hunting for Planetary Nebulae toward the Galactic Center