ИСТИНА

Imaging spectropolarimetry provides information about distribution of light polarization in astrophysical objects both in spectral and spatial domains. Polarization of the radiation is observed in a variety of astronomical objects: AGN and quasars, circumstellar envelopes of the symbiotic stars, supernova remnants, star-forming regions, planetary and protoplanetary nebulae. Polarization often strongly depends on the wavelength of light. By means of the spectral polarimetric observations we can obtain the information about the spatial structure of objects and magnetic fields in them...