Abstract
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.
This is a preview of subscription content, log in via an institution to check access.
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
References
Arp, H. 1966, ApJS, 14, 1
de Vancouleurs et al. 1991, Third Reference Catalog of Bright Galaxies (RC3)
Dupraz, C., & Combes, F. 1986, A&A, 166, 53
Hernquist, L., & Quinn, P. 1988, ApJ, 331, 682
Hernquist, L. & Quinn, P. 1989, ApJ, 342, 1
Thomson, R.C. 1991, MNRAS, 253, 256
Thomson, R.C. & Wright, A.E., 1990, MNRAS, 247, 122
Quinn, P. 1984, ApJ, 279, 596
Author information
Authors and Affiliations
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 1999 Springer Science+Business Media Dordrecht
About this paper
Cite this paper
Turnbull, A.J., Carter, D., Bridges, T.J., Thomson, R.C. (1999). Shell Formation in Ngc 474. In: Barnes, J.E., Sanders, D.B. (eds) Galaxy Interactions at Low and High Redshift. International Astronomical Union, vol 186. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-4665-4_40
Download citation
DOI: https://doi.org/10.1007/978-94-011-4665-4_40
Publisher Name: Springer, Dordrecht
Print ISBN: 978-0-7923-5833-6
Online ISBN: 978-94-011-4665-4
eBook Packages: Springer Book Archive