Nuclear activity in nearby galaxies
LC Ho - Annu. Rev. Astron. Astrophys., 2008 - annualreviews.org
A significant fraction of nearby galaxies show evidence of weak nuclear activity unrelated to
normal stellar processes. Recent high-resolution, multiwavelength observations indicate that …
normal stellar processes. Recent high-resolution, multiwavelength observations indicate that …
The relationship between luminosity and broad-line region size in active galactic nuclei
S Kaspi, D Maoz, H Netzer, BM Peterson… - The Astrophysical …, 2005 - iopscience.iop.org
We reinvestigate the relationship between the characteristic broad-line region size (R BLR)
and the Balmer emission-line, X-ray, UV, and optical continuum luminosities. Our study …
and the Balmer emission-line, X-ray, UV, and optical continuum luminosities. Our study …
The radius–luminosity relationship for active galactic nuclei: the effect of host-galaxy starlight on luminosity measurements. II. The full sample of reverberation-mapped …
We present high-resolution Hubble Space Telescope images of all 35 active galactic nuclei
(AGNs) with optical reverberation-mapping results, which we have modeled to create a …
(AGNs) with optical reverberation-mapping results, which we have modeled to create a …
The spectral energy distributions of low-luminosity active galactic nuclei
LC Ho - The Astrophysical Journal, 1999 - iopscience.iop.org
As a step toward elucidating the physical conditions in nearby active galaxies, this paper
presents spectral energy distributions (SEDs) of a sample of seven low-luminosity active …
presents spectral energy distributions (SEDs) of a sample of seven low-luminosity active …
Long-term optical variability properties of the Palomar—Green quasars
U Giveon, D Maoz, S Kaspi, H Netzer… - Monthly Notices of the …, 1999 - academic.oup.com
We present results from a monitoring programme of 42 quasars from the Palomar-Green
sample. The objects were observed for seven years at the Wise Observatory, as part of a …
sample. The objects were observed for seven years at the Wise Observatory, as part of a …
Nuclear luminosities and radio loudness of Seyfert nuclei
Historically, Seyfert nuclei have been considered to be radio-quiet active galactic nuclei
(AGNs). We question this widely held assumption by showing that the distribution of the …
(AGNs). We question this widely held assumption by showing that the distribution of the …
The nuclear reddening curve for active galactic nuclei and the shape of the infrared to X-ray spectral energy distribution
CM Gaskell, RW Goosmann… - The Astrophysical …, 2004 - iopscience.iop.org
We present extinction curves derived from the broad emission lines and continua of samples
of 72 radio-loud and 1018 radio-quiet active galactic nuclei (AGNs). The curves are …
of 72 radio-loud and 1018 radio-quiet active galactic nuclei (AGNs). The curves are …
[HTML][HTML] A study of the Baldwin effect in the IUE data set
AL Kinney, AR Rivolo… - … ), vol. 357, July 10, 1990, p …, 1990 - adsabs.harvard.edu
A study of the Baldwin effect in the IUE data set ADS Classic is now deprecated. It will be
completely retired in October 2019. This page will automatically redirect to the new ADS …
completely retired in October 2019. This page will automatically redirect to the new ADS …
Double-peaked broad emission lines in NGC 4450 and other LINERS
LC Ho, G Rudnick, HW Rix, JC Shields… - The Astrophysical …, 2000 - iopscience.iop.org
Spectra taken with the Hubble Space Telescope (HST) reveal that NGC 4450 emits Balmer
emission lines with displaced double peaks and extremely high velocity wings. This …
emission lines with displaced double peaks and extremely high velocity wings. This …
The X-ray spectra of high-luminosity active galactic nuclei observed by Ginga
OR Williams, MJL Turner, GC Stewart… - … Journal, Part 1 …, 1992 - adsabs.harvard.edu
Results are presented on the X-ray emission from 13 objects, observed by Ginga as part of a
spectral survey of bright quasars in the energy range 2-20 keV. The distribution of the power …
spectral survey of bright quasars in the energy range 2-20 keV. The distribution of the power …