B2 1521+28

B2 1521+28 is classfied as a low-luminosity radio galaxy with an elliptical host.^[4][3] Its surface brightness profile is excessive over the De Vaucouleurs's law model mainly in the external parts of the host galaxy.^[4] Imaging made with Hubble Space Telescope (HST), showed there is an unresolved nucleus located at the position of the galaxy core.^[5]

B2 1521+28 has a compact radio source. When observed with Very Large Array (VLA), the source contains a bright radio core with a radio spectrum found mainly either inverted or flat. In additional, it has a pair of two radio lobes that are asymmetric in terms of radio flux and also in extension from the position of the radio core. The lobe on the northern side displays marginal spectral gradients while the lobe on the southern side has a spectral index around the hotspot with it steepening. Both lobes also has polarization with depolarization ratios being 0.29 ± 0.05 for the northern lobe and 0.74 ± 0.05 for the southern lobe.^[6] There is also a weak hotspot located in the southern lobe with an increasing spectral index upon reaching outwards.^[7]

Observations found there is a radio jet present in B2 1521+28. Based on results, the jet is found to be one-sided.^[8] There are also several brightness knots present with the jet itself displaying a small amplitude oscillations in its main bright part. A major bending is observed towards the west direction which is subsequently followed by a counter-bend in the eastern direction. The spectral index of the jet is estimated to be 0.65 ± 0.05 from the core position by 20 kiloparsecs.^[6]

• B2 1521+48 on SIMBAD