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Ir optical bands hblrs - PowerPoint PPT Presentation

The Differences in the SEDs of Type 1 and Type 2 AGNs: Contributions from starbursts

The Differences in the SEDs of Type 1 and Type 2 AGNs: Contributions from starbursts. Xue-Bing Wu Collaborator: Ran Wang (Astronomy Department, Peking University) See also poster of Ran Wang. Content. Introduction AGN Data & SEDs Bolometric luminosity and nuclear AGN power

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Ir optical bands hblrs - PowerPoint PPT Presentation

The Differences in the SEDs of Type 1 and Type 2 AGNs: Contributions from starbursts