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On the Dynamics of very Flattened Ellipticals

Published online by Cambridge University Press:  25 May 2016

H. Dejonghe ,
V. de Bruyne ,
P. Vauterin  and
W.W. Zeilinger
H. Dejonghe
Affiliation:
Sterrenkundig Observatorium, Universiteit Gent, Krijgslaan 281, B-9000 Gent, Belgium
V. de Bruyne
Affiliation:
Sterrenkundig Observatorium, Universiteit Gent, Krijgslaan 281, B-9000 Gent, Belgium
P. Vauterin
Affiliation:
Sterrenkundig Observatorium, Universiteit Gent, Krijgslaan 281, B-9000 Gent, Belgium
W.W. Zeilinger
Affiliation:
Institut für Astronomie, Türkenschanzstraße 17, A–1180 Wien, Austria

Extract

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Our aim is to study the generic phase-space structure of flattened ellipticals by investigating a few typical cases. Here we report on the E4 elliptical NGC 4697.

The construction of 2-integral and 3-integral distribution functions asks for photometry and kinematic data. In the course of the data analysis, we additionally detected a nuclear dust lane at 3.4″ or 0.4 kpc from the centre, which could be confirmed with HST data. This was put to good use to constrain the inclination.

Type
Poster Papers
Information
Symposium - International Astronomical Union , Volume 171: New Light on Galaxy Evolution , 1996 , pp. 360
Copyright
Copyright © Kluwer 1996 

References

Binney, J.J., Davies, R.L. & Illingworth, G.D., 1990, ApJ, 361, 78 Google Scholar
Dejonghe, H., 1989, ApJ, 343, 113 Google Scholar
Dejonghe, H., De Bruyne, V., Vauterin, P., Zeilinger, W.W., A&A, in press Google Scholar