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Showing 1 to 10 of 10 for “"Quasare"”.

  1. Anwendung des Mikrogravitationslinseneffekts zur Untersuchung astronomischer Objekte

    … Arbeit werden die Spektren von drei gelinsten Quasare, die mit dem Potsdamer Multi Aperture Spectrophotometer (PMAS) erhalten wurden, auf Anzeichen für Mikrolensing untersucht. In den Spektren des Vierfachquasares HE 0435-1223 und des Doppelquasares HE 0047-1756 konnten Hinweise für …

    potsdam-diss Repository record for Anwendung des Mikrogravitationslinseneffekts zur Untersuchung astronomischer Objekte (opens in a new tab)

  2. Magnetic jets from accretion disks : field structure and X-ray emission

    … Sternen, stellaren schwarzen Löchern ('Mikro-Quasare'), Galaxien mit aktivem Kern (AGN) und wahrscheinlich auch mit dem beobachteten intensiven Aufblitzen von Gamma-Strahlung (Gamma Ray Bursts). Insbesondere hat sich gezeigt, dass die Jets der Mikro-Quasare wahrscheinlich als kleinskalige …

    potsdam-diss Repository record for Magnetic jets from accretion disks : field structure and X-ray emission (opens in a new tab)

  3. Cosmological applications of gravitational lensing

    In dieser Arbeit benutze ich den Gravitationslinseneffekt als ein Werkzeug, um zwei recht unterschiedliche kosmologische Fragestellungen zu bearbeiten: die Natur der dunklen Materie in Galaxienhalos und die Rotation des Universums. Zuerst untersuche ich den Mikrolinseneffekt in den …

    potsdam-diss Repository record for Cosmological applications of gravitational lensing (opens in a new tab)

  4. Demographics of supermassive black holes

    Supermassive black holes are a fundamental component of the universe in general and of galaxies in particular. Almost every massive galaxy harbours a supermassive black hole (SMBH) in its center. Furthermore, there is a close connection between the growth of the SMBH and the evolution of its host …

    potsdam-diss Repository record for Demographics of supermassive black holes (opens in a new tab)

  5. Constraining the UV background with the proximity effect

    After the epoch of reionisation the intergalactic medium (IGM) is kept at a high photoionisation level by the cosmic UV background radiation field. Primarily composed of the integrated contribution of quasars and young star forming galaxies, its intensity is subject to spatial and temporal …

    potsdam-diss Repository record for Constraining the UV background with the proximity effect (opens in a new tab)

  6. The AGN-host galaxy connection : new insights from the extended ionised gas

    Active Galactic Nuclei (AGN) are powered by gas accretion onto supermassive Black Holes (BH). The luminosity of AGN can exceed the integrated luminosity of their host galaxies by orders of magnitude, which are then classified as Quasi-Stellar Objects (QSOs). Some mechanisms are needed to trigger …

    potsdam-diss Repository record for The AGN-host galaxy connection : new insights from the extended ionised gas (opens in a new tab)

  7. Wechselwirkung von Gammastrahlung mit dem metagalaktischen Strahlungsfeld

    Im Rahmen dieser Arbeit wurden Effekte der Paarbildung durch Wechselwirkung von hochenergetischer Gammastrahlung mit dem metagalaktischen FIR-UV Strahlungsfeld (MRF) untersucht. Einerseits hat die Paarbildung Folgen f"ur die beobachteten Spektren aktiver Galaxienkerne, andererseits hat sie auch …

    wurz-thes Repository record for Wechselwirkung von Gammastrahlung mit dem metagalaktischen Strahlungsfeld (opens in a new tab)

  8. Detecting and understanding extragalactic Lyman α emission using 3D spectroscopy

    In this thesis we use integral-field spectroscopy to detect and understand of Lyman α (Lyα) emission from high-redshift galaxies. Intrinsically the Lyα emission at λ = 1216 Å is the strongest recombination line from galaxies. It arises from the 2p → 1s transition in hydrogen. In star-forming …

    potsdam-diss Repository record for Detecting and understanding extragalactic Lyman α emission using 3D spectroscopy (opens in a new tab)

  9. X-ray and optical properties of X-ray luminous active galactic nuclei

    Giacconi et al. (1962) discovered a diffuse cosmic X-ray background with rocket experiments when they searched for lunar X-ray emission. Later satellite missions found a spectral peak in the cosmic X-ray background at ~30 keV. Imaging X-ray satellites such as ROSAT (1990-1999) were able to resolve …

    potsdam-diss Repository record for X-ray and optical properties of X-ray luminous active galactic nuclei (opens in a new tab)

  10. The HI Lyman-alpha opacity at redshift 2.7 < z < 3.6

    Most of the baryonic matter in the Universe resides in a diffuse gaseous phase in-between galaxies consisting mostly of hydrogen and helium. This intergalactic medium (IGM) is distributed in large-scale filaments as part of the overall cosmic web. The luminous extragalactic objects that we can …

    potsdam-diss Repository record for The HI Lyman-alpha opacity at redshift 2.7 < z < 3.6 (opens in a new tab)