The detection of spiral arm modulation in the mass distribution of an optically flocculent galaxy
Ivanio PuerariDavid L. BlockBruce G. ElmegreenJay A. FrogelPaul B. Eskridge
所有作者
Ivanio PuerariDavid L. BlockBruce G. ElmegreenJay A. FrogelPaul B. Eskridge
文献摘要
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.