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We conduct a survey of low surface brightness (LSB) satellite galaxies aroundthe Local Volume massive spirals using long exposures with small amateurtelescopes. We identified 27 low and very low surface brightness objects aroundthe galaxies NGC,672, 891, 1156, 2683, 3344, 4258, 4618, 4631, and 5457situated within 10 Mpc from us, and found nothing new around NGC,2903, 3239,4214, and 5585. Assuming that the dwarf candidates are the satellites of theneighboring luminous galaxies, their absolute magnitudes are in the range of-8.6 > M_B > -13.3, their effective diameters are 0.4-4.7 kpc, and the averagesurface brightness is 26.1 mag/sq arcsec. The mean linear projected separationof the satellite candidates from the host galaxies is 73 kpc. Our spectroscopicobservations of two LSB dwarfs with the Russian 6-meter telescope confirm theirphysical connection to the host galaxies NGC,891 and NGC,2683.

New Low Surface Brightness Dwarf Galaxies Detected Around Nearby Spirals