Местоположение издательства:Bellingham, WA, United States
Первая страница:319
Последняя страница:319
Аннотация: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...