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

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dc.creatorPuerari, Ivanio
dc.creatorBlock, David L.
dc.creatorElmegreen, Bruce G.
dc.creatorFrogel, Jay A.
dc.creatorEskridge, Paul B.
dc.date2000-10-26
dc.date.accessioned2026-07-07T01:56:14Z
dc.date.available2026-07-07T01:56:14Z
dc.descriptionSpiral 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.
dc.description2 pages, 2 figures, to appear in ASP Conf. Ser. "Galaxy Disk and Disk Galaxies", Eds. J.G. Funes S.J. and E.M. Corsini (meeting held in Rome, June 12-16, 2000)
dc.identifierhttps://arxiv.org/abs/astro-ph/0010532
dc.identifierhttp://arxiv.org/abs/astro-ph/0010532
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/1923
dc.subjectAstrophysics
dc.titleThe detection of spiral arm modulation in the mass distribution of an optically flocculent galaxy
dc.typetext

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