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Documents Accretion High Energy Astrophysics [email protected]

Slide 1Accretion High Energy Astrophysics [email protected] http://www.mssl.ucl.ac.uk/ Slide 2 2 2.Accretion: Accretion by compact objects; Eddington luminosity limit; Emission…

Technology Alma observations of_feed_and_feedback_in_nearby_seyfert_galaxies

1. c ESO 2013Astronomy & Astrophysics manuscript no. nugas1 September 17, 2013ALMA observations of feeding and feedback in nearby Seyfert galaxies: an AGN-driven outflow…

Documents Chapter 15, Galaxies G alaxies come in different size and shape. In the previous chapter, we talked....

Slide 1 Chapter 15, Galaxies G alaxies come in different size and shape. In the previous chapter, we talked about how galaxies provide an environment for the stars to be…

Documents Imaging Quasars with Interferometry

Imaging Quasars with Interferometry Martin Elvis Harvard-Smithsonian Center for Astrophysics Why Study Quasars and AGN? Up to 1000 Galaxy Luminosities Visible to z > 6…

Documents NOTES: Active Galactic Nuclei (AGN) QUASARS: Radio Quasi-Stellar Objects. Maarten Schmidt examined.....

NOTES: Active Galactic Nuclei (AGN) QUASARS: Radio Quasi-Stellar Objects. Maarten Schmidt examined 3C273 (3C=Third Cambridge Catalog of Radio sources) and found its distance…

Documents Observations of AGN with MIDI or „How to cope with faint targets with MIDI“ EuroSummer School...

Observations of AGN with MIDI or „How to cope with faint targets with MIDI“ EuroSummer School Observation and data reduction with the VLTI Konrad R. W. Tristram MPIA…