Published October 2, 2003
| public
Book Section - Chapter
Mass Distributions in Early-Type Galaxy Halos
Chicago
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Abstract
One of the most promising avenues for determining the distribution of mass in the outer parts of early-type galaxies is through the kinematics of planetary nebulae (PNe). We have used new techniques and instrumentation on the WHT and the VLT to obtain velocities for hundreds of PNe around several nearby galaxies. We show simple mass models and describe more rigorous orbit modeling methods for the combined analysis of different dynamical constraints in galaxy halos.
Additional Information
© 2003 Springer-Verlag Berlin Heidelberg. First Online: 02 October 2003.Additional details
- Eprint ID
- 103827
- DOI
- 10.1007/10899892_19
- Resolver ID
- CaltechAUTHORS:20200610-141025148
- Created
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2020-06-10Created from EPrint's datestamp field
- Updated
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2021-11-16Created from EPrint's last_modified field
- Series Name
- ESO Astrophysics Symposia