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It has been suggested that the high metallicity generally observed in active galactic nuclei (AGNs) and quasars originates from ongoing star formation in the self-gravitating part of accretion disks a...
Observations of the Galactic Center (GC) have accumulated a multitude of "forensic" evidence indicating that several million years ago the center of the Milky Way galaxy was teaming with starforming a...
We have mapped the stellar and gaseous kinematics, as well as the emission-line flux distributions and ratios, from the inner 450pc radius of Mrk1157, using 2D near-IR spectra obtained with the Gemini...
Observational Overview of the Feeding of Active Galactic Nuclei。
The density of the narrow-line region of type 1 Active Galactic Nuclei。
Adaptive Optics Observations of Active Galactic Nuclei:Zooming into the Central Parsec Region。
The optical counterpart of sax j1808.4{3658 in quiescence:evidence of an active radio pulsar?
The nature of the very extended emission line regions associated with active galactic nuclei。
The broad line region in active galactic nuclei。
Several QSO pairs have been reported and their redshifts determined, where the two objects in each pair are located across an active galaxy. The usually accepted explanation of such occurrences is tha...
We present the BV light curves analysis of late-type, long-period stars 29 Dra, 12 Cam for the season 2005/2006, and shorter-period star II Peg for the same season. High latitude spots (alternativel...
Although we do not observe directly black holes in the Universe, their presence has been inferred in several astrophysical systems, from galactic to extragalactic scales. In this work, we will restric...

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