Abstract
The Bologna survey (Colla et al. 1970, 1972, 1973) does not represent a particularly new achievement since the first records refer to 1968. We will summarize here the main properties for a statistical use of the survey, the differential counts and the isotropy characteristic of this flux level, the latter being completely new.
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
Preview
Unable to display preview. Download preview PDF.
References
Colla, A. et al., 1970, Astron. Astrophys. Suppl. 1, 281.
Colla, A. et al., 1972, Astron. Astrophys. Suppl. 1.
Colla, A. et al., 1973, Astron. Astrophys. Suppl. 11, 291.
Pearson, T.F., 1975, Mon. Not. Roy. Astron. Soc. 171, 475.
Robertson, J.G., 1973, Aust. J. Phys. 26, 403.
Webster, A.S., 1976, Mon. Not. Roy. Astron. Soc. 175, 61.
Webster, A.S., 1976, Mon. Not. Roy. Astron. Soc. 175, 71.
Author information
Authors and Affiliations
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 1977 International Astronomical Union
About this chapter
Cite this chapter
Fanti, C., Lari, C. (1977). The Bologna Survey of Radio Sources at 408 MHz. In: Jauncey, D.L. (eds) Radio Astronomy and Cosmology. International Astronomical Union / Union Astronomique Internationale, vol 74. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-1260-7_4
Download citation
DOI: https://doi.org/10.1007/978-94-010-1260-7_4
Publisher Name: Springer, Dordrecht
Print ISBN: 978-90-277-0839-7
Online ISBN: 978-94-010-1260-7
eBook Packages: Springer Book Archive