Issue |
A&A
Volume 436, Number 2, June III 2005
|
|
---|---|---|
Page(s) | 417 - 426 | |
Section | Extragalactic astronomy | |
DOI | https://doi.org/10.1051/0004-6361:20042014 | |
Published online | 30 May 2005 |
Variability of optical Fe II complex in narrow-line Seyfert 1 galaxy NGC 4051
1
National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China e-mail: wjy@bao.ac.cn
2
National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China
3
Department of Astronomy, Beijing Normal University, Beijing 100875, China e-mail: xthe@bun.edu.cn
Received:
15
September
2004
Accepted:
24
January
2005
The variability of optical blends
in NGC 4051 is examined from spectra extracted from the AGN Watch
program.
In our analysis, the
complex are subtracted
and measured, with the following results. Firstly,
the
variations
were detected in NGC 4051 during a 3-year period.
The identified
variations
followed the variations in continuum closely.
Secondly, the EW of
is reported to increase with
rising continuum flux, which is consistent with previous
claims that there is no convincing Baldwin Effect
in optical
. Thirdly,
by comparing the variations of Hβ and
, we
find that
scales with continuum flux
as
, which is
significantly different from the theoretical expectations.
Finally, in six selected Seyferts, four out of five Narrow-Line Seyfert 1 galaxies
present positive correlation between
and the continuum flux.
The negative correlations are identified in the remaining two
objects that have relatively broad profiles of Hβ (
).
We argue that the difference of electron density of broad line clouds and/or variability
behavior of incident high-energy radiation can explain the dichotomy in
variability behavior of
.
Key words: galaxies: active / galaxies: individual: NGC 4051 / galaxies: quasars: emission lines
© ESO, 2005
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