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Improving the triaxial bulge model of M31

By Simon Berman and Laurent Loinard


There is growing evidence that spiral galaxies in which no bar is easily seen on optical or infrared images, nonetheless, have triaxial bulges. Twisting of the inner isophotes and misalignments between the disk and the bulge majo

Topics: Accepted. Received, in original form
Year: 2002
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