Astronomy and Astrophysics – Astrophysics
Scientific paper
1998-10-20
Astronomy and Astrophysics
Astrophysics
18 pages, 22 figures, accepted for publication in MNRAS
Scientific paper
10.1046/j.1365-8711.1999.02210.x
We present new dynamical models of the S0 galaxy N3115, making use of the available published photometry and kinematics as well as of two-dimensional TIGER spectrography. We first examined the kinematics in the central 40 arcsec in the light of two integral f(E,J) models. Jeans equations were used to constrain the mass to light ratio, and the central dark mass whose existence was suggested by previous studies. The even part of the distribution function was then retrieved via the Hunter & Qian formalism. We thus confirmed that the velocity and dispersion profiles in the central region could be well fit with a two-integral model, given the presence of a central dark mass of ~10^9 Msun. However, no two integral model could fit the h_3 profile around a radius of 25 arcsec where the outer disc dominates the surface brightness distribution. Three integral analytical models were therefore built using a Quadratic Programming technique. These models showed that three integral components do indeed provide a reasonable fit to the kinematics, including the higher Gauss-Hermite moments. Again, models without a central dark mass failed to reproduce the observed kinematics in the central arcseconds. This clearly supports the presence of a nuclear black hole of at least 6.5 10^8 Msun in the centre of NGC 3115. These models were finally used to estimate the importance of the dark matter in the outer part of NGC 3115, suggested by the flat stellar rotation curve observed by Capaccioli et al. (1993).
Bacon Roland
Dejonghe Herwig
Emsellem Eric
No associations
LandOfFree
Dynamical models of NGC 3115 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Dynamical models of NGC 3115, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Dynamical models of NGC 3115 will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-372980