Astronomy and Astrophysics – Astrophysics – Cosmology and Extragalactic Astrophysics
Scientific paper
2010-03-24
Astronomy and Astrophysics
Astrophysics
Cosmology and Extragalactic Astrophysics
19 pages, 3 figures, 3 tables, accepted for publication in ApJ
Scientific paper
After recent sensitivity upgrades at the Keck Interferometer (KI), systematic interferometric 2um studies of the innermost dust in nearby Seyfert nuclei are within observational reach. Here, we present the analysis of new interferometric data of NGC 4151, discussed in context of the results from recent dust reverberation, spectro-photometric and interferometric campaigns. The complete data set gives a complex picture, in particular the measured visibilities from now three different nights appear to be rather insensitive to the variation of the nuclear luminosity. KI data alone indicate two scenarios: the K-band emission is either dominated to ~90% by size scales smaller than 30mpc, which falls short of any dust reverberation measurement in NGC 4151 and of theoretical models of circum-nuclear dust distributions. Or contrary, and more likely, the K-band continuum emission is dominated by hot dust (>= 1300K) at linear scales of about 50mpc. The linear size estimate varies by a few tens of percent depending on the exact morphology observed. Our interferometric, deprojected centro-nuclear dust radius estimate of 55+-5mpc is roughly consistent with the earlier published expectations from circum-nuclear, dusty radiative transfer models, and spectro-photometric modeling. However, our data do not support the notion that the dust emission size scale follows the nuclear variability of NGC 4151 as a R_dust \propto L_nuc^0.5 scaling relation. Instead variable nuclear activity, lagging, and variable dust response to illumination changes need to be combined to explain the observations.
Elitzur Moshe
Ghez Andrea M.
Herbst Tom M.
Malkan Matt A.
Pott Jorg-Uwe
No associations
LandOfFree
Luminosity-variation independent location of the circum-nuclear, hot dust in NGC 4151 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Luminosity-variation independent location of the circum-nuclear, hot dust in NGC 4151, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Luminosity-variation independent location of the circum-nuclear, hot dust in NGC 4151 will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-555499