Access

You are not currently logged in.

Access your personal account or get JSTOR access through your library or other institution:

login

Log in to your personal account or through your institution.

If You Use a Screen Reader

This content is available through Read Online (Free) program, which relies on page scans. Since scans are not currently available to screen readers, please contact JSTOR User Support for access. We'll provide a PDF copy for your screen reader.

ON THE GALAXIES IN THE DIRECTION OF TON 256 AND B 264

JOHN N. BAHCALL and NETA A. BAHCALL
Publications of the Astronomical Society of the Pacific
Vol. 82, No. 487 (June 1970), pp. 721-729
Stable URL: http://www.jstor.org/stable/40674896
Page Count: 9
  • Read Online (Free)
  • Subscribe ($19.50)
  • Cite this Item
Since scans are not currently available to screen readers, please contact JSTOR User Support for access. We'll provide a PDF copy for your screen reader.
ON THE GALAXIES IN THE DIRECTION OF TON 256 AND B 264
Preview not available

Abstract

Evidence is presented which suggests that the QSO Ton 256 could be in a cluster of galaxies with the same redshift as the QSO. In order to facilitate redshift determinations, accurate positions, magnitude estimates, and a finding chart are given for the brightest galaxies that are the most likely candidates for membership in a cluster containing Ton 256. Similar measurements are provided for the galaxies in the cluster of galaxies containing the QSO B 264.

Page Thumbnails

  • Thumbnail: Page 
721
    721
  • Thumbnail: Page 
722
    722
  • Thumbnail: Page 
723
    723
  • Thumbnail: Page 
724
    724
  • Thumbnail: Page 
725
    725
  • Thumbnail: Page 
726
    726
  • Thumbnail: Page 
727
    727
  • Thumbnail: Page 
728
    728
  • Thumbnail: Page 
729
    729