Abstract
The study of the relations between the radio continuum emission of spirals and other global properties (e.g.HI content, colours, Hα emission strengths, infrared emission, arm classification), which are know to be probably different in different environments, can be of aid in understanding the nature of the radio continuum emission. In the present study we examine a sample of nearby spirals (V0 < 3000Km/s).
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Giuricin, G., Mardirossian, F., Mezzetti, M. (1989). Nearby Spiral Galaxies: Optical and Radio Properties. In: Caffo, M., Fanti, R., Giacomelli, G., Renzini, A. (eds) Astronomy, Cosmology and Fundamental Physics. Astrophysics and Space Science Library, vol 155. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-0965-6_37
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DOI: https://doi.org/10.1007/978-94-009-0965-6_37
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