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A new insight on galaxy formation from infrared surveys |
What: |
A new insight on galaxy formation from infrared surveys
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Who: |
Dr. David Elbaz |
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When: |
Tuesday Morning,Nov.04th,10:00 a.m. |
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Where: |
Room 327, Office Block, 2 West Beijing Road (PMO, CAS)
Welcome to attend
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abstract
Some major issues concerning how galaxies formed have emerged during recent years. Massive galaxies formed earlier in an apparently anti-hierarchical way ("downsizing"). The growth of supermassive black holes (SMBH) through accretion appears to be related to that of stars in galaxies, still, it is commonly believed that active nuclei quenched star formation during the recent history of the Universe. Most of the black hole growth took place in obscured environments, such as star formation, we will see how deep infrared surveys, such as GOODS, the Great Observatories Origins Deep Survey, changed our vision of the history of dust obscured star formation and SMBH growth. One of the solutions proposed to explain the origin of the "downsizing" would be that the environment too acts stops the star formation activity in galaxies, we will address this issue thanks to the most complete spectroscopic sample of galaxies. The Herschel satellite is scheduled to be launched on April 12, 2009, hence very soon, we will briefly present its major extragalactic programs.
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Copyright? Purple Mountain Observatory, CAS, No.10 Yuanhua Road, Qixia District, Nanjing 210023, China
Phone: 0086 25 8333 2000 Fax: 8333 2091 http://english.pmo.cas.cn |
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