Integral-field observations of centaurus a nucleus

ESO ASTROPHY SYMP (2007) 277-279

Authors:

D Krajnovic, R Sharp, N Thatte

Abstract:

We observed the nuclear region of Centaurus A in the J band with CIRPASS, mounted on GEMINI South telescope. Here we present the preliminary results focusing on the kinematic structure of the gas disk and present a simple model determining its kinematic orientation and inclination as well as an estimate of the mass of the central black hole.

Integral-field spectroscopy of Centaurus A nucleus

Monthly Notices of the Royal Astronomical Society 374 (2007) 385-398

Authors:

N Thatte, Krajnovic, Davor, Sharp, Rob

Physics, and faith are worth debating

PHYSICS WORLD 20:12 (2007) 23-23

Authors:

Andrew Briggs, Gavin Dalton, Paul Ewart, Andrew Steane, Justin Wark, William Phillips

Practical implementation of the complex wavefront modulation model for optical alignment - art. no. 66170N

P SOC PHOTO-OPT INS 6617 (2007) N6170-N6170

Authors:

H Lee, GB Dalton, IAJ Tosh, SW Kim

Abstract:

We discuss the implementation of the complex wavefront modulation model in practical optical alignment procedures and present its interim results. This modulation model describes the relation between the alignment state and the wavefront of a system, both are expressed in mathematical complex quantities. It addresses the importance of the coupled inter-element alignment effect to the resultant system wavefront. We utilise this effect in order to extract the alignment state of a system from measured optical wavefronts. We demonstrate the method's practical applicability to the real optical alignment procedure by showing alignment simulations of a centered three-mirror system.

SAURON observations of sa bulges: The formation of a kinematically decoupled core in NGC 5953

ESO ASTROPHY SYMP (2007) 111-115

Authors:

J Falcon-Barroso, R Bacon, M Bureau, M Cappellari, RL Davies, PT de Zeeuw, E Emsellem, K Fathi, D Krajnovic, H Kuntschner, RM McDermid, RF Peletier, M Sarzi

Abstract:

We present results from our ongoing effort to understand the nature and evolution of nearby galaxies using the SAURON integral-field spectrograph. In this proceeding we focus on the study of the particular case formed by the interacting galaxies NGC 5953 and NGC 5954. We present stellar and gas kinematics of the central regions of NGC5953. We use a simple procedure to determine the age of the stellar populations in the central regions and argue that we may be witnessing the formation of a kinematically decoupled component (hereafter KDC) from cold gas being acquired during the ongoing interaction with NGC 5954.