Determination of instabilities in the NGC 5427 circumnuclear disk

Details Determination of instabilities in the NGC 5427 circumnuclear disk Determination of instabilities in the NGC 5427 circumnuclear disk

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009rmxac..35s.302p&link_type=abstract

XII Latin American IAU Regional Meeting (Eds. G. Magris, G. Bruzual, & L. Carigi) Revista Mexicana de Astronomía y Astrofísica (

Astronomy and Astrophysics

Astronomy

Scientific paper

We have applied photometric methods to calculate the Toomre parameter of
the circumnuclear region of NGC 5427 using visible and near-infrared
Hubble Space Telescope images. We study the types of instability that
appear in the dynamics, and determine the morphology of this
circumnuclear region, from the point of view of a density wave scenario.

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