Arm width as a function of absolute luminosity for bc, C spiral galaxies

Details Arm width as a function of absolute luminosity for bc, C spiral galaxies Arm width as a function of absolute luminosity for bc, C spiral galaxies

May 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982a%26a...109..336b&link_type=abstract

Astronomy and Astrophysics, vol. 109, no. 2, May 1982, p. 336-339. Research supported by the University of the Orange Free Stat

Astronomy and Astrophysics

Astrophysics

10

Correlation Coefficients, Galactic Structure, Luminous Intensity, Spiral Galaxies, Statistical Correlation, Disk Galaxies, Morphology, Width

Scientific paper

Linear widths of the spiral arms of 27 Shapley-Ames type bc, c galaxies
are presented, along with the distance and corrected absolute blue
magnitude of the parent galaxy. A strong correlation of the latter value
with arm width is found, with a correlation coefficient of 0.89.
Successively brighter bc, c spirals have wider arms.

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