activity
20052009
most citedThe starburst-AGN connection: the role of young stellar populations in fueling supermassive black holes

38 citations · 81 across the 5 of their papers we have counts for

collaborators

6 papers

astro-ph.CO200915 cited

Evolution of gaseous disk viscosity driven by supernova explosion in star-forming galaxies at high redshift

Jian-Min Wang, Chang-Shuo Yan, Yan-Rong Li +5

Motivated by Genzel et al.'s observations of high-redshift star-forming galaxies, containing clumpy and turbulent rings or disks, we build a set of equations describing the dynamic…

astro-ph.GA200938 cited

The starburst-AGN connection: the role of young stellar populations in fueling supermassive black holes

Y. -M. Chen, J. -M. Wang, C. -S. Yan +2

Tracing the star formation history in circumnuclear regions (CNRs) is a key step towards understanding the starburst-AGN connection. However, bright nuclei outshining the entire ho…

astro-ph200824 cited

Spins of the supermassive black hole in M87: new constraints from TeV observations

Jian-Min Wang, Yan-Rong Li, Jain-Cheng Li +1

The rapid TeV ray variability detected in the well-known nearby radio galaxy M87 implies an extremely compact emission region (5-10 Schwarzschild radii) near the horizon of the…

astro-ph20064 cited

INTEGRAL and XMM-Newton observations towards the unidentified MeV source GRO J1411-64

Diego F. Torres, Shu Zhang, Olaf Reimer +9

The COMPTEL unidentified source GRO J1411-64 was observed by INTEGRAL, and its central part, also by XMM-Newton. The data analysis shows no hint for new detections at hard X-rays.…

astro-ph2006

A quasi periodic signal with ultra low frequency discovered in V0332+53?

Shu Zhang, Diego F. Torres, JinLu Qu

The reported likely QPO is found to be an instrumental effect, which was never clarified in any INTEGRAL related literatures. The paper should therfore be withdrawn.

astro-ph2005

Discovery of new quasi-periodic oscillations in the X-ray transient source V~0332+53

J. L. Qu, S. Zhang, L. Song +1

We report the discovery of a new quasi-period oscillation (QPO) at 0.22 Hz, centered on the source spin frequency of the high mass X-ray binary system V~0332+53 when the source was…