Abstract
A complete search on KPNO 4-m plates has been undertaken in order to determine the whole observable part of the cluster luminosity function of the late-type spiral galaxy NGC 2403. Automatic procedures have been used for object detection and analysis, and then selection criteria, based on geometric and photometric properties, have been applied in order to define the sample of cluster candidates.
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
References
Battistini, P., Bonoli, F., Frederici, L., Fusi Pecci, F. and Kron, R. G. 1984 Astron. Astrophys. 130, 162.
Malagnini, M. L., Pasian, F., Pucillo, M. and Santin, P. 1985 Astron. Astrophys. 144, 49.
Tammann, G. A. and Sandage, A. 1986 Astrophys. J. 151, 825.
Author information
Authors and Affiliations
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 1988 IAU
About this paper
Cite this paper
Malagnini, M.L., Santin, P., Bonoli, F., Frederici, L., Fusi Pecci, F., Kron, R.G. (1988). A Search for Globular Cluster Candidates in NGC 2403. In: Grindlay, J.E., Davis Philip, A.G. (eds) The Harlow-Shapley Symposium on Globular Cluster Systems in Galaxies. International Astronomical Union / Union Astronomique Internationale, vol 126. Springer, Dordrecht. https://doi.org/10.1007/978-94-015-1104-9_96
Download citation
DOI: https://doi.org/10.1007/978-94-015-1104-9_96
Publisher Name: Springer, Dordrecht
Print ISBN: 978-90-277-2665-0
Online ISBN: 978-94-015-1104-9
eBook Packages: Springer Book Archive