Supermassive black holes from OASIS and SAURON integral-field kinematics

Michele Cappellari*, R. Bacon, Roger L. Davies, P. T. De Zeeuw, Eric Emsellem, Jesús Falcón-Barroso, Davor Krajnović, Harald Kuntschner, Richard M. McDermid, Reynier F. Peletier, Marc Sarzi, Remco C E Van Den Bosch, Glenn Van De Ven

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

Abstract

Supermassive black holes are a key element in our understanding of how galaxies form. Most of the progress in this very active field of research is based on just ~30 determination of black hole masses, accumulated over the past decade. We illustrate how integral-field spectroscopy, and in particular our OASIS modeling effort can help improve the current situation.

Original languageEnglish
Pages (from-to)215-218
Number of pages4
JournalProceedings of the International Astronomical Union
Volume3
Issue numberS245
DOIs
Publication statusPublished - Jul 2007
Externally publishedYes

Keywords

  • Black hole physics
  • Galaxies: elliptical and lenticular
  • Galaxies: kinematics and dynamics
  • Galaxies: nuclei

Fingerprint Dive into the research topics of 'Supermassive black holes from OASIS and SAURON integral-field kinematics'. Together they form a unique fingerprint.

Cite this