Abstract
The Revised Shapley-Ames Catalog (Sandage & Tamman, 1981) contains 335 spiral galaxies brighter than BT = 12. A subsample of these galaxies with δ ≥ -25° and total flux densities at 1.49 GHz (Condon, 1987) above 10 mJy were observed at λ2.8 cm using the 100-m radio telescope of the MPIfR Bonn. Depending on the expected flux density and extent of the source two observational methods were used: cross-scanning and mapping. In total, radio flux densities of 192 galaxies have been derived (Niklas et al., 1995). Additionally, a literature search was made in order to get flux densities at other frequencies.
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References
Sandage, A., Tammann, G.A. 1981, A Revised Shapley-Ames Catalog of Bright Galaxies (Washington, D.C.: Carnegie Institution of Washington)(RSA)
Condon, J. 1987, ApJS, 65, 465
Niklas, S., Klein, U., Braine, J., Wielebinski, R. 1995, A&AS, 113
Kennicutt, R.C., Kent, S.M. 1983, ApJ, 88, 1094
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© 1996 Springer Science+Business Media Dordrecht
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Niklas, S., Wielebinski, R., Klein, U., Braine, J. (1996). Results of a Radio Continuum Survey of Spiral Galaxies at 10.55 GHz. In: Bender, R., Davies, R.L. (eds) New Light on Galaxy Evolution. International Astronomical Union / Union Astronomique Internationale, vol 171. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-0229-9_136
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DOI: https://doi.org/10.1007/978-94-009-0229-9_136
Publisher Name: Springer, Dordrecht
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