Supermassive black holes from OASIS and SAURON integral-field kinematics

Bibcode
2008IAUS..245..215C
DOI
10.1017/S1743921308017687
Cappellari, Michele; Bacon, R.; Davies, Roger L.; de Zeeuw, P. T.; Emsellem, Eric; Falcón-Barroso, Jesús; Krajnović, Davor; Kuntschner, Harald; McDermid, Richard M.; Peletier, Reynier F.; Sarzi, Marc; van den Bosch, Remco C. E.; van de Ven, Glenn
Referencia bibliográfica

Formation and Evolution of Galaxy Bulges, Proceedings of the International Astronomical Union, IAU Symposium, Volume 245, p. 215-218

Fecha de publicación:
7
2008
Número de autores
13
Número de autores del IAC
0
Número de citas
21
Número de citas referidas
21
Descripción
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.
Tipo
Sin árbitro
Física de los agujeros negros
Galaxias

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