Gas Kinematics from Hα line in NGC 4151 (Sergeev, 1994)

Details Gas Kinematics from Hα line in NGC 4151 (Sergeev, 1994) Gas Kinematics from Hα line in NGC 4151 (Sergeev, 1994)

Nov 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996ycat..80710189s&link_type=abstract

VizieR On-line Data Catalog: J/AZh/71/189. Originally published in: 1994AZh....71..189S

Physics

Active Gal. Nuclei, Spectroscopy

Scientific paper

The nucleus spectra of the Seyfert galaxy NGC 4151 obtained in 1988-1991 were analyzed in order to study the profile variability of the Ha line resulting from ionizing continuum flux variations. At the time of this galaxy monitoring, the response of the integral flux of the Ha line was almost linear and the average profile shape did not change by more than 5%. (2 data files).

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