The detection of spiral arm modulation in the mass distribution of an optically flocculent galaxy

Details The detection of spiral arm modulation in the mass distribution of an optically flocculent galaxy The detection of spiral arm modulation in the mass distribution of an optically flocculent galaxy

2000-10-26

arxiv.org/abs/astro-ph/0010532v1

Astronomy and Astrophysics

Astrophysics

2 pages, 2 figures, to appear in ASP Conf. Ser. "Galaxy Disk and Disk Galaxies", Eds. J.G. Funes S.J. and E.M. Corsini (meetin

Scientific paper

Spiral arm modulation in NGC 4062 (an optical flocculent) is detected for the
first time; the Fourier spectra of NGC 4062 and NGC 5248 (a classic grand
design in optical images) are almost identical.

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