Axisymmetric Structures in Galactic Nuclei - Theoretical Consequences

Details Axisymmetric Structures in Galactic Nuclei - Theoretical Consequences Axisymmetric Structures in Galactic Nuclei - Theoretical Consequences

Aug 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007jena.confr..59s&link_type=abstract

"JENAM-2007, "Our non-stable Universe", held 20-25 August 2007 in Yerevan, Armenia. Abstract book, p. 59-59"

Physics

Scientific paper

Structures (either gaseous or stellar) of considerable mass and axially symmetric to the first approximation are observed in many galactic nuclei. In my contribution I will discuss two different aspects of their presence: (i) their perturbing gravitational potential may influence motion of stars in a characteristic way, with possible observational consequences; (ii) due to their deduced stability they can serve as probes of the external gravitational field.

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