Counter-rotating gaseous disks in the 'Evil Eye' galaxy NGC4826

Details Counter-rotating gaseous disks in the 'Evil Eye' galaxy NGC4826 Counter-rotating gaseous disks in the 'Evil Eye' galaxy NGC4826

Dec 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992natur.360..442b&link_type=abstract

Nature (ISSN 0028-0836), vol. 360, no. 6403, p. 442-444.

Other

67

Counter Rotation, Galactic Rotation, Galactic Structure, Interacting Galaxies, Interstellar Gas, Spiral Galaxies, Elliptical Galaxies, Galactic Evolution, Star Formation

Scientific paper

The discovery of two counterrotating gaseous disks in the otherwise
normal early-type spiral NGC4826 is reported. This is the most disklike
galaxy in which any kinematic substructure has yet been found. This
discovery raises the possibility that even spiral galaxies may have
undergone a significant degree of structural evolution due to mergers.

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