Ja. Garciabarreto et al., HIGH-FREQUENCY RADIO-CONTINUUM OBSERVATIONS OF BARRED SPIRAL GALAXIES, Revista Mexicana de Astronomia y Astrofisica, 25(1), 1993, pp. 31-38
We have determined the central radio continuum fluxes at 6.3 and 2.8 c
m from a subset of barred spiral galaxies from the Shapley Ames Catalo
g with the 100-m radiotelescope in Effelsberg. We calculated the spect
ral indices for the galaxies detected and we can see a weak correlatio
n between flat spectral index and dust temperature calculated from IRA
S fluxes, that is, T(d) greater-than-or-equal-to 30-degrees-K for gala
xies having alpha6.3/20 greater-than-or-equal-to -0.75. The radio cont
inuum at both frequencies and the far-infrared fluxes are strongly cor
related.