Mass distributions in early-type galaxy halos

  • AJ Romanowsky*
  • , NG Douglas
  • , K Kuijken
  • , MR Merrifield
  • , M Arnaboldi
  • , KC Freeman
  • , K Taylor
  • *Corresponding author for this work

Research output: Chapter in Book/Report/Conference proceedingConference contributionAcademicpeer-review

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.

Original languageEnglish
Title of host publicationMASS OF GALAXIES AT LOW AND HIGH REDSHIFT
EditorsT Bender, A Renzini
Place of PublicationBERLIN
PublisherSpringer
Pages72-73
Number of pages2
ISBN (Print)3-540-00205-7
Publication statusPublished - 2003
EventWorkshop on the Mass of Galaxies at Low and High Redshift - , Italy
Duration: 24-Oct-200126-Oct-2001

Publication series

NameESO ASTROPHYSICS SYMPOSIA
PublisherSPRINGER-VERLAG BERLIN

Other

OtherWorkshop on the Mass of Galaxies at Low and High Redshift
Country/TerritoryItaly
Period24/10/200126/10/2001

Keywords

  • ELLIPTIC GALAXIES

Fingerprint

Dive into the research topics of 'Mass distributions in early-type galaxy halos'. Together they form a unique fingerprint.

Cite this