Astrophysics and Space Science

, Volume 269, Issue 0, pp 427–430

What is the True Fraction of Barred Spiral Galaxies?

Authors

  • Paul B. Eskridge
    • Department of AstronomyThe Ohio State University
  • Jay A. Frogel
    • Department of AstronomyThe Ohio State University
Article

DOI: 10.1023/A:1017025820201

Cite this article as:
Eskridge, P.B. & Frogel, J.A. Astrophysics and Space Science (1999) 269: 427. doi:10.1023/A:1017025820201

Abstract

We have determined the fraction of barred galaxies in the H-band for a statistically well-defined sample of 186 spirals. At H, 56% of our sample is strongly barred, 16% is weakly barred, and only 27% is unbarred. The RC3 and the Carnegie Atlas of Galaxies both classify roughly 30% of our sample as strongly barred. Thus strong bars are nearly twice as prevalent in the H-band as in the optical. Roughly 40% of the galaxies in our sample that are classified as unbarred in the RC3 show evidence for a bar in the H-band; for the Carnegie Atlas the fraction is roughly 60%. We find no significant trend in bar fraction as a function of morphology, in either the optical or H-band.

Copyright information

© Kluwer Academic Publishers 1999