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Faint Features of Galaxies revealed by the Digital Co-addition of Schmidt Plates
Published online by Cambridge University Press: 12 April 2016
Abstract
We have digitally co-added eight IIIa-J/GG395 UKST plates centred on the IC 4296 cluster of galaxies. The factor of increase in S/N in the co-added array enables galaxy profiles to be followed, and filamentary and diffuse features to be detected, down to bj surface brightnesses of 28 mag arcsec−2. Examples of warped disks, shells, trails, diffuse IGM and extended haloes revealed by this technique are discussed and illustrated.
- Type
- VII. Digitisation of Schmidt Data
- Information
- International Astronomical Union Colloquium , Volume 148: The Future Utilisation of Schmidt Telescopes , 1995 , pp. 200 - 206
- Copyright
- Copyright © Astronomical Society of the Pacific 1995
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