Hostname: page-component-586b7cd67f-dlnhk Total loading time: 0 Render date: 2024-11-26T01:40:07.898Z Has data issue: false hasContentIssue false

Shell Formation in NGC 474

Published online by Cambridge University Press:  25 May 2016

A.J. Turnbull
Affiliation:
University of Hertfordshire, Hatfield, Herts, UK
D. Carter
Affiliation:
Liverpool John Moores, Byrom Street, Liverpool, UK
T.J. Bridges
Affiliation:
Royal Greenwich Observatory, Cambridge, UK
R. C. Thomson
Affiliation:
University of Hertfordshire, Hatfield, Herts, UK

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We present broad band photometry (B and R) of the classic shell galaxy NGC 474. Preliminary results indicate that the shells have a similar colour to and follow the same trend of colour with radius as the underlying galaxy.

Type
Mergers & Remnants
Copyright
Copyright © Kluwer 1999 

References

Arp, H. 1966, ApJS, 14, 1 Google Scholar
de Vancouleurs, et al. 1991, Third Reference Catalog of Bright Galaxies (RC3) CrossRefGoogle Scholar
Dupraz, C., & Combes, F. 1986, A&A, 166, 53 Google Scholar
Hernquist, L., & Quinn, P. 1988, ApJ, 331, 682 CrossRefGoogle Scholar
Hernquist, L. & Quinn, P. 1989, ApJ, 342, 1 Google Scholar
Thomson, R.C. 1991, MNRAS, 253, 256 Google Scholar
Thomson, R.C. & Wright, A.E., 1990, MNRAS, 247, 122 Google Scholar
Quinn, P. 1984, ApJ, 279, 596 CrossRefGoogle Scholar