A conventional explanation for the axial ratio anomalies of bar-within-ring galaxies

Details A conventional explanation for the axial ratio anomalies of bar-within-ring galaxies A conventional explanation for the axial ratio anomalies of bar-within-ring galaxies

Oct 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ap%26ss.115..195o&link_type=abstract

Astrophysics and Space Science, Volume 115, Issue 1, pp.195-196

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

Previously reported excesses of high b/a(disk) and b/a(ring) values for
bar-within-ring galaxies are found to be due to a selection effect.
Three other anomalous properties appear to remain problematic for flat
disk models.

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