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

doi:10.1017/S1743921308017687

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 journal › Article › peer-review

3 Citations (Scopus)

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 language	English
Pages (from-to)	215-218
Number of pages	4
Journal	Proceedings of the International Astronomical Union
Volume	3
Issue number	S245
DOIs	https://doi.org/10.1017/S1743921308017687
Publication status	Published - Jul 2007
Externally published	Yes

Keywords

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

Access to Document

10.1017/S1743921308017687

Cite this

Cappellari, M., Bacon, R., Davies, R. L., De Zeeuw, P. T., Emsellem, E., Falcón-Barroso, J., Krajnović, D., Kuntschner, H., McDermid, R. M., Peletier, R. F., Sarzi, M., Van Den Bosch, R. C. E., & Van De Ven, G. (2007). Supermassive black holes from OASIS and SAURON integral-field kinematics. Proceedings of the International Astronomical Union, 3(S245), 215-218. https://doi.org/10.1017/S1743921308017687

@article{793d8bdd8f1343c98f93d1483485be1d,

title = "Supermassive black holes from OASIS and SAURON integral-field kinematics",

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 \textasciitilde{}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.",

keywords = "Black hole physics, Galaxies: elliptical and lenticular, Galaxies: kinematics and dynamics, Galaxies: nuclei",

author = "Michele Cappellari and R. Bacon and Davies, \{Roger L.\} and \{De Zeeuw\}, \{P. T.\} and Eric Emsellem and Jes{\'u}s Falc{\'o}n-Barroso and Davor Krajnovi{\'c} and Harald Kuntschner and McDermid, \{Richard M.\} and Peletier, \{Reynier F.\} and Marc Sarzi and \{Van Den Bosch\}, \{Remco C E\} and \{Van De Ven\}, Glenn",

year = "2007",

month = jul,

doi = "10.1017/S1743921308017687",

language = "English",

volume = "3",

pages = "215--218",

journal = "Proceedings of the International Astronomical Union",

issn = "1743-9213",

publisher = "Cambridge University Press (CUP)",

number = "S245",

}

Cappellari, M, Bacon, R, Davies, RL, De Zeeuw, PT, Emsellem, E, Falcón-Barroso, J, Krajnović, D, Kuntschner, H, McDermid, RM, Peletier, RF, Sarzi, M, Van Den Bosch, RCE & Van De Ven, G 2007, 'Supermassive black holes from OASIS and SAURON integral-field kinematics', Proceedings of the International Astronomical Union, vol. 3, no. S245, pp. 215-218. https://doi.org/10.1017/S1743921308017687

TY - JOUR

T1 - Supermassive black holes from OASIS and SAURON integral-field kinematics

AU - Cappellari, Michele

AU - Bacon, R.

AU - Davies, Roger L.

AU - De Zeeuw, P. T.

AU - Emsellem, Eric

AU - Falcón-Barroso, Jesús

AU - Krajnović, Davor

AU - Kuntschner, Harald

AU - McDermid, Richard M.

AU - Peletier, Reynier F.

AU - Sarzi, Marc

AU - Van Den Bosch, Remco C E

AU - Van De Ven, Glenn

PY - 2007/7

Y1 - 2007/7

N2 - 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.

AB - 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.

KW - Black hole physics

KW - Galaxies: elliptical and lenticular

KW - Galaxies: kinematics and dynamics

KW - Galaxies: nuclei

UR - https://www.scopus.com/pages/publications/46749119512

U2 - 10.1017/S1743921308017687

DO - 10.1017/S1743921308017687

M3 - Article

AN - SCOPUS:46749119512

SN - 1743-9213

VL - 3

SP - 215

EP - 218

JO - Proceedings of the International Astronomical Union

JF - Proceedings of the International Astronomical Union

IS - S245

ER -

Supermassive black holes from OASIS and SAURON integral-field kinematics

Abstract

Keywords

Access to Document

Other files and links

Fingerprint

Cite this