Is there a relationship between AGN and star formation in IR-bright AGNs?
Title: Is there a relationship between AGN and star formation in IR-bright AGNs?
Speaker: 戴昱(NAOC)
Time: 3 pm, NOV. 01(Thursday)
Location: Lecture Hall, 3rd floor
Abstract: In this talk, I will review the importance and tips learned from AGN modeling, based on our recent work on the relationship between AGN and star formation in a sample of X-ray selected, infrared AGNs. We compared several AGN SED models and the effect of AGN removal in the infrared based on their X-ray information, and found significant AGN contributions to the infrared luminosities and corresponding star formation rate estimates. I will then review the AGN-star formation relation on a multi-parameter space and how different parameters and sample selections affect the observed correlation. Finally, I will report the constant ratio discovered between the star formation rate and the black hole mass accretion rate, and their implications on the gas supply, galaxy formation history, and galaxy evolutionary models.
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Speaker:9:30am, August 01th, Tuesday
Time:Yan Gong (Max-Planck-Institute for Radio Astronomy)
Location:Middle conference room, 3rd floor
Speaker:9:30 am July 27th (Thursday)
Time:Junhao Liu (East Asian Observatory)
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Speaker:Wednesday, July 26th 3:00pm
Time:Dr. Pinghui Huang (黄平辉)
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Location:1715
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Speaker:1:30 pm July 6th (Thursday)
Time:Prof. Wen-Ping Chen (National Central University)
Location:Lecture Hall, 3rd floor