Integral-Field Observations of Centaurus A Nucleus

2009 ◽  
pp. 277-279
Author(s):  
D. Krajnović ◽  
R. Sharp ◽  
N. Thatte
Keyword(s):  
Field Observations ◽  
Integral Field ◽  
Centaurus A

scholarly journals The mass of the black hole in Centaurus A from SINFONI AO-assisted integral-field observations of stellar kinematics

2009 ◽  
Vol 394 (2) ◽  
pp. 660-674 ◽  
Author(s):  
Michele Cappellari ◽  
N. Neumayer ◽  
J. Reunanen ◽  
P. P. van der Werf ◽  
P. T. de Zeeuw ◽  
...  
Keyword(s):  
Black Hole ◽  
Field Observations ◽  
Stellar Kinematics ◽  
Integral Field ◽  
Centaurus A

scholarly journals Stars and gas in the inner parts of galaxies seen in SAURON integral field observations

2007 ◽  
Vol 51 (1-2) ◽  
pp. 29-33 ◽  
Author(s):  
R.F. Peletier ◽  
K. Fathi ◽  
E.L. Allard ◽  
J.H. Knapen ◽  
M. Sarzi ◽  
...  
Keyword(s):  
Field Observations ◽  
Inner Parts ◽  
Integral Field

scholarly journals Feeding Versus Feedback in AGNs from Near-Infrared IFU Observations: The Case of Mrk 1066

2009 ◽  
Vol 5 (S267) ◽  
pp. 405-405
Author(s):  
Rogemar A. Riffel ◽  
Thaisa Storchi-Bergmann
Keyword(s):  
Spatial Resolution ◽  
Central Region ◽  
Near Infrared ◽  
Galactic Plane ◽  
Seyfert Galaxy ◽  
Active Galaxies ◽  
Molecular Gas ◽  
Field Observations ◽  
Ionized Gas ◽  
Integral Field

Previous studies of the central region of active galaxies show that the molecular and ionized gas have distinct kinematics and flux distributions, with the former dominated by quiescent kinematics characteristic of rotation in the galactic plane and the latter with more disturbed kinematics and apparently extending to larger galactic latitudes. These results suggest that the molecular gas can be a tracer of the feeding of the AGN and the ionized gas a tracer of its feedback (e.g., Riffel et al. 2009, 2008, 2006; Storchi-Bergmann et al. 2009a, b). In the present study we use Gemini NIFS integral field observations of the inner 700×700 pc2 of the Seyfert galaxy Mrk 1066 at a spatial resolution of ~ 35 pc to investigate if the above scenario is also valid for this galaxy.

scholarly journals The central planetary nebulae populations of external galaxies with SAURON

2011 ◽  
Vol 7 (S283) ◽  
pp. 283-286
Author(s):  
Marc Sarzi
Keyword(s):  
Planetary Nebulae ◽  
Stellar Populations ◽  
Field Observations ◽  
Horizontal Branch ◽  
Early Type ◽  
Luminosity Functions ◽  
External Galaxies ◽  
Nuclear Regions ◽  
Integral Field

AbstractThanks to SAURON integral-field observations we uncovered the planetary nebulae (PNe) populations inhabiting the central and nuclear regions of our galactic neighbours M32 and M31, respectively, and discuss the significant differences between their corresponding PNe luminosity functions in light of the properties of their parent stellar populations. In particular, we conclude that the lack of bright PNe in the nuclear regions of M31 is likely linked to the nearly Solar value for the stellar metallicity, consistent with previous suggestions that a larger metallicity would bias the horizontal-branch (HB) populations toward bluer colors, leading to fewer red HB stars capable of producing PNe and more blue HB stars that instead could contribute to the far-UV flux observed in metal-rich early-type galaxies and, incidentally, in the nucleus of M31.

Integral field observations of damped Lyman-α galaxies

2004 ◽  
Vol 325 (2) ◽  
pp. 124-127 ◽  
Author(s):  
L. Christensen ◽  
S.F. Sánchez ◽  
K. Jahnke ◽  
T. Becker ◽  
A. Kelz ◽  
...  
Keyword(s):  
Field Observations ◽  
Integral Field

The contrast performance of the NIRSpec micro shutters and its impact on NIRSpec integral field observations

2018 ◽  
Author(s):  
Catarina Alves de Oliveira ◽  
Stephan M. Birkmann ◽  
Torsten Böker ◽  
Elena Puga ◽  
Timothy D. Rawle ◽  
...  
Keyword(s):  
Field Observations ◽  
Integral Field

Integral Field Observations of a Distant Cluster

2009 ◽  
pp. 397-400
Author(s):  
D. Vergani ◽  
C. Balkowski ◽  
V. Cayatte ◽  
H. Flores ◽  
F. Hammer ◽  
...  
Keyword(s):  
Field Observations ◽  
Distant Cluster ◽  
Integral Field
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