The possible origin of the mini-spiral in the nuclear disk of the Galaxy as a result of the super-reflection instability

Details The possible origin of the mini-spiral in the nuclear disk of the Galaxy as a result of the super-reflection instability The possible origin of the mini-spiral in the nuclear disk of the Galaxy as a result of the super-reflection instability

Nov 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009arep...53..969f&link_type=abstract

Astronomy Reports, Volume 53, Issue 11, pp.969-975

Astronomy and Astrophysics

Astronomy

Galactic Center, Bar, Circumnuclear Matter, And Bulge

Scientific paper

It is shown that the mini-spiral in the nuclear disk of the Galaxy could
arise as a result of super-reflection instability in the disk. This
instability develops at a break in the profile of the disk rotation. The
structure of the perturbation obtained via numerical modeling is
visually similar to the observed mini-spiral.

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