A low upper-mass limit for the central black hole in the late-type galaxy NGC 4414
We present our mass estimate of the central black hole in the isolated spiral galaxy NGC 4414. Using natural guide star adaptive optics assisted observations with the Gemini Near-Infrared Integral Field Spectrometer (NIFS) and the natural seeing Gemini MultiObject Spectrographs-North (GMOS), we deri...
Autori principali: | Thater, S, Krajnovic, D, Bourne, M, Cappellari, M, de Zeeuw, T, Emsellem, E, Magorrian, J, McDermid, R, Sarzi, M, van de Ven, G |
---|---|
Natura: | Journal article |
Lingua: | English |
Pubblicazione: |
EDP Sciences
2016
|
Documenti analoghi
Documenti analoghi
-
SAURON dynamical modeling of NGC 2974
di: Krajnovic, D, et al.
Pubblicazione: (2004) -
Six new supermassive black hole mass determinations from adaptive-optics assisted SINFONI observations
di: Thater, S, et al.
Pubblicazione: (2019) -
Dynamical modelling of stars and gas in NGC 2974: determination of mass-to-light ratio, inclination and orbital structure using the Schwarzschild method
di: Krajnovic, D, et al.
Pubblicazione: (2005) -
Two channels of supermassive black hole growth as seen on the galaxies mass-size plane
di: Krajnović, D, et al.
Pubblicazione: (2017) -
Determination of masses of the central black holes in NGC 524 and 2549 using laser guide star adaptive optics
di: Krajnovic, D, et al.
Pubblicazione: (2009)