University of Hertfordshire

The kinematics of Core and Cusp galaxies: comparing HST imaging and integral-field observations

Research output: Chapter in Book/Report/Conference proceedingConference contribution

  • J. Falcon-Barroso
  • R. Bacon
  • M. Cappellari
  • R.L. Davies
  • P.T. de Zeeuw
  • E. Emsellem
  • D. Krajnovic
  • H. Kuntschner
  • R.M. McDermid
  • R.F. Peletier
  • Marc Sarzi
  • G. van de Ven
View graph of relations
Original languageEnglish
Title of host publicationThe Impact of HST on European Astronomy
EditorsF. Duccio Macchetto
PublisherSpringer
Pages127-132
ISBN (Print)9789048133994, 9048133998
Publication statusPublished - 2010

Abstract

In this proceeding we look at the relationship between the photometric nuclear properties of early-type galaxies from Hubble Space Telescope imaging and their overall kinematics as observed with the SAURON integral-field spectrograph. We compare the inner slope of their photometric profiles and the Slow/Fast rotator classes, defined by the amplitude of a newly defined λR parameter, to show that slow rotators tend to be more massive systems and display shallower inner profiles and fast rotators steeper ones. It is important to remark, however, that there is not a one-to-one relationship between the two photometric and kinematic groups.

Notes

Proceedings of the 41st ESLAB Symposium. Copyright Springer [Full text of this chapter is not available in the UHRA]

ID: 146740