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image/svg+xml Jakob Voss, based on art designer at PLoS, modified by Wikipedia users Nina and Beao Closed Access logo, derived from PLoS Open Access logo. This version with transparent background. http://commons.wikimedia.org/wiki/File:Closed_Access_logo_transparent.svg Jakob Voss, based on art designer at PLoS, modified by Wikipedia users Nina and Beao Astronomische Nachri...arrow_drop_down
image/svg+xml Jakob Voss, based on art designer at PLoS, modified by Wikipedia users Nina and Beao Closed Access logo, derived from PLoS Open Access logo. This version with transparent background. http://commons.wikimedia.org/wiki/File:Closed_Access_logo_transparent.svg Jakob Voss, based on art designer at PLoS, modified by Wikipedia users Nina and Beao
Astronomische Nachrichten
Article . 2005 . Peer-reviewed
License: Wiley Online Library User Agreement
Data sources: Crossref
image/svg+xml Jakob Voss, based on art designer at PLoS, modified by Wikipedia users Nina and Beao Closed Access logo, derived from PLoS Open Access logo. This version with transparent background. http://commons.wikimedia.org/wiki/File:Closed_Access_logo_transparent.svg Jakob Voss, based on art designer at PLoS, modified by Wikipedia users Nina and Beao
Astronomische Nachrichten
Article . 2007 . Peer-reviewed
License: Wiley Online Library User Agreement
Data sources: Crossref
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Active Galactic Nuclei

Authors: Martin Haas; Peter Biermann; Rolf Chini; Jochen Heidt; Wolfram Kollatschny; Helmut Meusinger; Ralf Siebenmorgen;

Active Galactic Nuclei

Abstract

AbstractD01 Direct evidence of the receding ‘torus’ around active galactic nuclei of FRII radio galaxies and quasarsD02 Infrared emission from a clumpy and dusty torus around AGND03 Size and properties of AGN narrow–line regions from emission–line diagnosticsD04 Structural Variability of Intraday Variable SourcesD05 Stability of self‐gravitating accretion disks in galactic centersD06 Supermassive Binary Black Holes in AGND07 The extreme flare in III Zw 2: Evolution of a radio jet in a Seyfert galaxyD08 Radio Linear and Circular Polarization from M81*D09 A fundamental relation between Supermassive Black Holes and Dark Matter HaloesD10 Hunting for radio‐quiet BL Lacs – the 2dF BL Lac surveyD11 The Eddington limit in accretion discsD12 Molecular Tori in AGN: A search using excited states of OHD13 The X‐Ray Properties of Radio‐Loud Core‐Dominated AGN: The 2 cm‐X‐SampleD14 The X‐Ray Properties of Radio‐Loud Core‐Dominated AGN: Extension to the High Redshift RegimeD15 Line Profile Variability in AGND16 Jet Superwind InteractionD17 Radio Interferometric Observations of AGN – Probing the Nucleus of M87 with 20 Schwarzschild radii resolutionD18 The ISO–2MASS AGN surveyD19 Supermassive binary black holes driving the activity of galactic nucleiD20 Proton acceleration at quasi‐perpendicular shocks: A case study for Active Galactic NucleiD21 Super‐luminal shocks in Active Galactic NucleiD22 Unconventional quasars from the variability and proper motion surveyD23 Radio observations of starburst and AGN activity in Ultraluminous Infrared GalaxiesD24 Kinematics in Active Galactic Nuclei at Parsec Scales: the VLBA 2cm SurveyD25 Three‐dimensional models of clumpy tori in Seyfert galaxiesD26 Silicate emission in active galaxies ‐ From LINERs to QSOsD27 Discovery of 10 µm silicate emission in quasars. – Evidence of the AGN unification scheme.D28 Near‐IR adaptive optics imaging of luminous infrared galaxiesD29 Interferometric observations of the Circinus galaxy with MIDID30 Infrared Interferometry of the Seyfert Galaxy NGC 1068

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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
0
Average
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