H-alpha Profile as an Effective Instrument for Study of Variability of Seyfert Galaxies

Details H-alpha Profile as an Effective Instrument for Study of Variability of Seyfert Galaxies H-alpha Profile as an Effective Instrument for Study of Variability of Seyfert Galaxies

Aug 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007jena.confe..52g&link_type=abstract

"JENAM-2007, "Our non-stable Universe", held 20-25 August 2007 in Yerevan, Armenia. Abstract book, p. 52-52"

Physics

Scientific paper

An efficiency of spectral observations of Seyfert galaxies in the red wavelength range is discussed. As the H-alpha emission is one of the strongest lines in the spectrum of AGN its observation is accessible even for the small instruments. At the same time variations of H-alpha profile reflect the corresponding changes of the central source of ionization.

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