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Active Galactic Nuclei

Overview of attention for book
Cover of 'Active Galactic Nuclei'

Table of Contents

  1. Altmetric Badge
    Book Overview
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    Chapter 159 Emission-line spectra and the nature of active galactic nuclei
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    Chapter 160 Emission line regions in active galactic nuclei: A unified view
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    Chapter 161 Emission-line region structure from variability studies
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    Chapter 162 UV and optical spectroscopy of NGC 5548
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    Chapter 163 The circumnuclear environment of the nearby non-interacting Seyfert galaxies NGC 5273 and NGC 3516
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    Chapter 164 Long-slit spectroscopy of star-burst galaxies
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    Chapter 165 Voyager far UV observations of Markarian 509
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    Chapter 166 High resolution study of NGC 4151
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    Chapter 167 Long-slit echelle spectrograms of Seyfert galaxy nuclei
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    Chapter 168 Double peaked broad line profiles — edge on accretion disks or double quasar nuclei?
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    Chapter 169 OJ287 as a binary system
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    Chapter 170 Line profiles and the kinematics of the narrow-line region
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    Chapter 171 Reddening of narrow line regions
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    Chapter 172 Ultraviolet and optical spectra of broad-line radio galaxies
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    Chapter 173 Long slit CCD observations of active and normal galaxies
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    Chapter 174 Imaging spectrophotometry of ionized gas in active galaxies
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    Chapter 175 Some spectroscopic properties of mass-ejecting and radio-loud quasars
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    Chapter 176 Infrared spectroscopy of NGC 1068
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    Chapter 177 Dust and emission-line asymmetries in active galaxies
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    Chapter 178 Spectropolarimetry and the structure of active galactic nuclei
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    Chapter 179 Spectropolarimetry of “narrow-line Seyfert 1s”
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    Chapter 180 Evidence for thermal emission components in highly polarized quasars
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    Chapter 181 The shape of the ultraviolet continuum of quasars
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    Chapter 182 A search for IRAS AGN
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    Chapter 183 Nuclear activity in warm IRAS galaxies
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    Chapter 184 An optical and radio survey of southern radio galaxies
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    Chapter 185 A study of Sérsic-Pastoriza galaxies
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    Chapter 186 Infrared emission and tidal interactions of spiral galaxies
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    Chapter 187 The optical variability of selected blazars
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    Chapter 188 Long-term monitoring of a large sample of active galactic nuclei
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    Chapter 189 The long term optical variability of PKS 2201 + 044
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    Chapter 190 A photometric investigation of the optical variability of Markarian 501
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    Chapter 191 The optical variability of Arakelian 120, 1977–1987
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    Chapter 192 Observations of the 1987 outburst of AO 0235+164
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    Chapter 193 A complete spectral analysis of the flare of the quasar 3C 273
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    Chapter 194 Broad line variations of Seyfert galaxies
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    Chapter 195 Effect of pulsed variations of the ionizing continuum on the narrow line region
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    Chapter 196 Observations and interpretation of the multifrequency continua of AGN and QSOs
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    Chapter 197 Theory of AGN continuum radiation
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    Chapter 198 Model for the continuum emission of active galactic nuclei
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    Chapter 199 Fitting multi-wavelength continuum of AGN with improved accretion disk models
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    Chapter 200 Accretion-disk modelling of the optical-UV spectrum of quasars
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    Chapter 201 Synthesis of accretion disk and nonthermal source models for AGN
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    Chapter 202 Effects of self-gravity in AGNs
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    Chapter 203 Mass and length scale of black holes in quasars and active galactic nuclei
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    Chapter 204 X-ray spectra of active galaxies
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    Chapter 205 Clues to the X-ray emission mechanisms in flat radio spectrum AGNs
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    Chapter 206 X-ray timing of active galactic nuclei
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    Chapter 207 X-ray and optical studies of iras selected AGN
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    Chapter 208 Leakage of UHE photons from AGNs: Production of X-ray and γ-ray halos within 10–30 KPC
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    Chapter 209 Radiation dynamics and pair creation in AGN accretion shocks
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    Chapter 210 Thermal comptonization in compact sources and the cosmic X-ray background
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    Chapter 211 Radio sources: Small scale structure
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    Chapter 212 The internal conditions of parsec-scale relativistic jets
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    Chapter 213 The nuclear jet in M87
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    Chapter 214 European VLBI network observations of Seyfert Nuclei
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    Chapter 215 VLBI observations of the radio lobe spiral galaxy, NGC3079
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    Chapter 216 Compact steep spectrum radio sources
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    Chapter 217 The CM-wavelength fluxes and linear polarizations of BL Lac objects
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    Chapter 218 Large scale radio structures
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    Chapter 219 Triple radio structure in the “double-nucleus” galaxy Markarian 266
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    Chapter 220 VLA observation of the M87 jet and small scale jet structures
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    Chapter 221 Extended optical line emission in powerful radio galaxies
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    Chapter 222 The interaction of radio jets with the narrow line region in Seyfert galaxies
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    Chapter 223 Optical continuum shapes of extragalactic radio jets
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    Chapter 224 The interaction of relativistic jets in AGNs with the ambient radiation field
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    Chapter 225 A circuit analogy for active galactic nuclei
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    Chapter 226 A model for quasi-one-dimensional narrow jets
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    Chapter 227 Two-and-one-half dimensional models of radio jets
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    Chapter 228 Linear size versus redshift and linear size versus power for extended extragalactic radio sources
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    Chapter 229 Evolution of radio jets in galactic halos and the intergalactic medium
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    Chapter 230 AGNS in clusters of galaxies and the bootes void
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    Chapter 231 Space distribution and luminosity function of quasars
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    Chapter 232 A preliminary examination of redshift and luminosity characteristics for APM survey quasars
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    Chapter 233 The evolution of active galactic nuclei: A multi-mass model
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    Chapter 234 Evolution of low luminosity quasars
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    Chapter 235 Evolutionary sequence of Seyfert galaxies
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    Chapter 236 Multiple QSO images with arcminute splittings
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    Chapter 237 Relativistic beaming, luminosity functions, and cosmology
Overall attention for this book and its chapters
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About this Attention Score

  • In the top 25% of all research outputs scored by Altmetric
  • High Attention Score compared to outputs of the same age (90th percentile)
  • High Attention Score compared to outputs of the same age and source (92nd percentile)

Mentioned by

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1 blog

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mendeley
2 Mendeley
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Title
Active Galactic Nuclei
Published by
ADS, January 2006
DOI 10.1007/3-540-19492-4
ISBNs
978-3-54-019492-7, 978-3-54-039304-7
Editors

Miller, H. Richard, Wiita, Paul J.

Mendeley readers

Mendeley readers

The data shown below were compiled from readership statistics for 2 Mendeley readers of this research output. Click here to see the associated Mendeley record.

Geographical breakdown

Country Count As %
Unknown 2 100%

Demographic breakdown

Readers by professional status Count As %
Student > Bachelor 1 50%
Other 1 50%
Readers by discipline Count As %
Earth and Planetary Sciences 1 50%
Physics and Astronomy 1 50%
Attention Score in Context

Attention Score in Context

This research output has an Altmetric Attention Score of 9. This is our high-level measure of the quality and quantity of online attention that it has received. This Attention Score, as well as the ranking and number of research outputs shown below, was calculated when the research output was last mentioned on 04 January 2023.
All research outputs
#3,919,343
of 26,017,215 outputs
Outputs from ADS
#2,181
of 27,022 outputs
Outputs of similar age
#13,630
of 177,322 outputs
Outputs of similar age from ADS
#23
of 311 outputs
Altmetric has tracked 26,017,215 research outputs across all sources so far. Compared to these this one has done well and is in the 83rd percentile: it's in the top 25% of all research outputs ever tracked by Altmetric.
So far Altmetric has tracked 27,022 research outputs from this source. They typically receive a little more attention than average, with a mean Attention Score of 5.1. This one has done particularly well, scoring higher than 90% of its peers.
Older research outputs will score higher simply because they've had more time to accumulate mentions. To account for age we can compare this Altmetric Attention Score to the 177,322 tracked outputs that were published within six weeks on either side of this one in any source. This one has done particularly well, scoring higher than 90% of its contemporaries.
We're also able to compare this research output to 311 others from the same source and published within six weeks on either side of this one. This one has done particularly well, scoring higher than 92% of its contemporaries.