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

Bruce G. Elmegreen (3); David L. Block (2); Ivanio Puerari (1); Jay A. Frogel (4); Paul B. Eskridge (4) ((1) INAOE - Mexico; (2) University of Witwatersrand - South Africa; (3) IBM Research Division; The Ohio State University; T.J. Watson Research Centre; USA); USA; (4) Dept of Astronomy

arxiv: astro-ph/0010532 · v1 · submitted 2000-10-26 · 🌌 astro-ph

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

Ivanio Puerari (1) , David L. Block (2) , Bruce G. Elmegreen (3) , Jay A. Frogel (4) , Paul B. Eskridge (4) ((1) INAOE - Mexico; (2) University of Witwatersrand - South Africa; (3) IBM Research Division , T.J. Watson Research Centre , USA; (4) Dept of Astronomy , The Ohio State University

show 1 more author

USA)

This is my paper

classification 🌌 astro-ph

keywords flocculentmodulationopticalspiralalmostclassicdesigndetected

0 comments

read the original abstract

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.

This paper has not been read by Pith yet.

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

discussion (0)