Feeding and feedback of super-massive black holes: inflows and outflows in the two nearest galactic nuclei
Abstract:
Studies of nearby galactic nuclei hold promise for understanding the interaction and evolution of the central super-massive black hole and its environment, which is crucial for understanding galaxy evolution in general. In the first part of this talk, I will present a study of cool gas in the nuclear region of the Andromeda galaxy (M31), based on recently available HST images tracing dust extinction. I will discuss the morphology and fine structures of the dusty gas under sub-parsec resolutions, the extinction law in a spatially-resolved fashion, and implications on the physical regulation of the circumnuclear ISM. In the second part, I will present new evidence for a long-sought jet emanating from the Galactic Center Black Hole, known as Sgr A*, based on recent Chandra and VLA observations.
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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)
Location:Middle conference room, 3rd floor
Speaker:Wednesday, July 26th 3:00pm
Time:Dr. Pinghui Huang (黄平辉)
Location:Middle conference room, 3rd floor
Speaker:7月14日,星期五,上午10点
Time:闫大海(云南大学)
Location:1715
Speaker:3:00 pm July 13th (Thursday)
Time:Shuang Zhou (University of Nottingham)
Location:Lecture Hall, 3rd floor
Speaker:1:30 pm July 6th (Thursday)
Time:Prof. Wen-Ping Chen (National Central University)
Location:Lecture Hall, 3rd floor