'Bolometric luminosity' diaporamas de présentation

Multi-wavelength Observations of Galaxies at z>~2

Multi-wavelength Observations of Galaxies at z>~2. Mauro Giavalisco (UMass) + The GOODS Team + The COSMOS Team. Color selection at z~2: BzK galaxies. BzK selection: 1.4<z<2.5. BzK selection more general than UV selection (LBG). It is reddening independent and it includes:

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The Obscured Growth Phase of Black Holes in Distant Massive Galaxies

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The Evolution of AGN Obscuration

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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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UV to Mid-IR SEDs of Low Redshift Quasars

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Schematic History of the Universe

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Detection of Star-Planet Interaction with Future X-ray Missions

Detection of Star-Planet Interaction with Future X-ray Missions. Scott J. Wolk I. Pillitteri, O. Cohen, V. Kashyap, C. Lisse, J. Drake. What is Star Planet Interaction?. Cuntz et al. 2000. Could the Planet really Matter?. HD 189733b 1G (1/2 Jupiter). HD 189733 40G. Cohen et al. 2011.

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Co-accreting disk/corona system in AGNs with double-peaked emission lines

Co-accreting disk/corona system in AGNs with double-peaked emission lines. XuYun. outline. 1.The properties of AGNs with double-peaked emission lines. 2.Our models. Co-accreting disk/corona system. 3.Other models. 4.Our research method. 5. Final result.

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Collaborators: Chuck Steidel (Caltech), Max Pettini (IoA), Alice Shapley (UCLA),

Naveen Reddy (Hubble Fellow, NOAO). Dust Obscuration and Metallicity at z~2: Implications for the Selection and Stellar Populations of High-Redshift Galaxies. Collaborators: Chuck Steidel (Caltech), Max Pettini (IoA), Alice Shapley (UCLA), Dawn Erb (UCSB).

271 views • 10 slides