The nucleus of the Seyfert galaxy NGC 4151 - A search for 1-day variability in the broad emission-line components

Details The nucleus of the Seyfert galaxy NGC 4151 - A search for 1-day variability in the broad emission-line components The nucleus of the Seyfert galaxy NGC 4151 - A search for 1-day variability in the broad emission-line components

Aug 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984pazh...10..574b&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 10, Aug. 1984, p. 574-582) Soviet Astronomy Letters (ISSN 0360-0327), vol. 10, July-Aug

Astronomy and Astrophysics

Astronomy

2

Astronomical Spectroscopy, Emission Spectra, Galactic Nuclei, Seyfert Galaxies, Balmer Series, Galactic Radiation, H Beta Line, Spectral Line Width

Scientific paper

A portion of the spectrum of NGC 4151 Seyfert galaxy nucleus was
observed during 9 nights of the periods March 31 - April 6 and May 29 -
June 3, 1983. A (1 - 2) - day variability of the broad components of the
lines mentioned seems to exist. Increasing of the whole Hβ blue
wing during the course of 2 months was observed.

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