R. Perna et T. Di Matteo, Synchrotron emission from hot accretion flows and the cosmic microwave background anisotropy, ASTROPHYS J, 542(1), 2000, pp. 68-73
Current estimates of number counts of radio sources in the frequency range
in which the most sensitive cosmic microwave background (CMB) experiments a
re carried out significantly underrepresent sources with strongly inverted
spectra. Hot accretion flows around supermassive black holes in the nuclei
of nearby galaxies are expected to produce inverted radio spectra by therma
l synchrotron emission. We calculate the temperature fluctuations and power
spectra of these sources in the Planck Surveyor 30 GHz energy channel, whe
re their emission is expected to peak. We find that their potential contrib
ution is generally comparable to the instrumental noise, and approaches the
CMB anisotropy level at small angular scales. Forthcoming missions, which
will provide a large statistical sample of inverted-spectra sources, will b
e crucial for determining the distribution of hot accretion flows in nearby
quiescent galactic nuclei. Detection of these sources in different frequen
cy channels will help constrain their spectral characteristics, and hence t
heir physical properties.