Received: 2011-8-8
Accepted: 2011-8-15
Published Online: 2017-3-23
Published in Print: 2011-9-1
© 2017
Articles in the same Issue
- Photometry and Classification of Stars in the Direction of the Dark Cloud TGU 619 in Cepheus. II. Interstellar Extinction and Cloud Distance
- A New Dynamical Parameter for the Study of Sticky Orbits in a 3D Galactic Model
- Preface
- Scorpio On the 6m Telescope: Current State and Perspectives for Spectroscopy of Galactic and Extragalactic Objects
- FIR/Submm Spectroscopy with Herschel: First Results from the VNGS and H-Atlas Surveys
- High Redshift Quasars, Emission Lines and ‘Cloudy’
- Variability of Double-Peaked Emission Lines in AGNs as a Probe of the Broad-Line Region Structure
- Off-Axis Variability of AGNs: A New Paradigm for Broad Lines and Continuum Emitting Regions
- Accretion Disk Structure and Kinematics of the Broad Line Regions in Selected AGN
- A Photo-Ionization Method for Black Hole Mass Estimation in Quasars
- Microlensing-Based Studies of the Unresolved Structure of AGNs and the Composition of Lensing Galaxies
- The Starburst – AGN Connection: a Critical Review
- The Case for Two Quasar Populations
- Equivalent width Measurements in Optical Spectra of Galaxies in Local Clusters: Hints On the Star Formation History in Clusters
- Optical Emission Lines and the X-Ray Properties of Type 1 Seyfert Galaxies
- The Complex Broad Absorption Line Profiles in a Sample of QSO Spectra
- A Complex Stellar Line-of-Sight Velocity Distribution in the Lenticular Galaxy NGC 524
- Observations of the Galaxy NGC 3077 in the Narrow-Band [S II] and Hα Filters
- The Reliability of [C II] as a Star Formation Rate Indicator
- Influence of Black Hole Spin on the Shape of the Fe Kα Spectral Line: The Case of 3C 405
- Hints on the Broad Line Region Structure of Quasars at High and Low Luminosities
- Spectral Monitoring of AGN: Preliminary Results for Ark 564 and Arp 102B
- Influence of Microlensing on Spectral Anomalies of the Lensed Objects
- Gas Motion Mapping for Three Seyfert Galaxies
- AGN Dusty Tori as a Clumpy Two-Phase Medium: the 10 μm Silicate Feature
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BY-NC-ND 4.0
Articles in the same Issue
- Photometry and Classification of Stars in the Direction of the Dark Cloud TGU 619 in Cepheus. II. Interstellar Extinction and Cloud Distance
- A New Dynamical Parameter for the Study of Sticky Orbits in a 3D Galactic Model
- Preface
- Scorpio On the 6m Telescope: Current State and Perspectives for Spectroscopy of Galactic and Extragalactic Objects
- FIR/Submm Spectroscopy with Herschel: First Results from the VNGS and H-Atlas Surveys
- High Redshift Quasars, Emission Lines and ‘Cloudy’
- Variability of Double-Peaked Emission Lines in AGNs as a Probe of the Broad-Line Region Structure
- Off-Axis Variability of AGNs: A New Paradigm for Broad Lines and Continuum Emitting Regions
- Accretion Disk Structure and Kinematics of the Broad Line Regions in Selected AGN
- A Photo-Ionization Method for Black Hole Mass Estimation in Quasars
- Microlensing-Based Studies of the Unresolved Structure of AGNs and the Composition of Lensing Galaxies
- The Starburst – AGN Connection: a Critical Review
- The Case for Two Quasar Populations
- Equivalent width Measurements in Optical Spectra of Galaxies in Local Clusters: Hints On the Star Formation History in Clusters
- Optical Emission Lines and the X-Ray Properties of Type 1 Seyfert Galaxies
- The Complex Broad Absorption Line Profiles in a Sample of QSO Spectra
- A Complex Stellar Line-of-Sight Velocity Distribution in the Lenticular Galaxy NGC 524
- Observations of the Galaxy NGC 3077 in the Narrow-Band [S II] and Hα Filters
- The Reliability of [C II] as a Star Formation Rate Indicator
- Influence of Black Hole Spin on the Shape of the Fe Kα Spectral Line: The Case of 3C 405
- Hints on the Broad Line Region Structure of Quasars at High and Low Luminosities
- Spectral Monitoring of AGN: Preliminary Results for Ark 564 and Arp 102B
- Influence of Microlensing on Spectral Anomalies of the Lensed Objects
- Gas Motion Mapping for Three Seyfert Galaxies
- AGN Dusty Tori as a Clumpy Two-Phase Medium: the 10 μm Silicate Feature