output
19972026
Showing 2010 · astro-ph.HEShow all

15 papers · 2 filters

astro-ph.HE2010★ 16 cited

RXTE/ASM and Swift/BAT Observations of Spectral Transitions in Bright X-ray Binaries in 2005-2010

Jing Tang, Wenfei Yu, Zhen Yan

We have studied X-ray spectral state transitions that can be seen in the long- term monitoring light curves of bright X-ray binaries from the All-Sky Monitor (ASM) on board the Ros…

astro-ph.HE2010★ 6 cited

Phase Drifts of Sub-pulses during the 2004 Giant Flare of SGR 1806-20 and Settling of the Magnetic Fields

Yi Xing, Wenfei Yu

We analyzed the observations of SGR 1806-20 performed with the \textit{Rossi X-ray Timing Explorer} (RXTE) during its 2004 giant flare. We studied the phase evolution of the sub-pu…

astro-ph.HE2010★ 54 cited

On the Origin of Ultraviolet Emission and the Accretion Model of Low-luminosity AGNs

Zhaolong Yu, Feng Yuan, Luis Ho

Low-luminosity active galactic nuclei (LLAGNs) are generally believed to be powered by an inner radiatively inefficient, advection-dominated accretion flow (ADAF), an outer truncat…

astro-ph.HE2010★ 19 cited

Magnetothermal and magnetorotational instabilities in hot accretion flows

De-Fu Bu, Feng Yuan, James M Stone

In a hot, dilute, magnetized accretion flow, the electron mean-free path can be much greater than the Larmor radius, thus thermal conduction is anisotropic and along magnetic field…

astro-ph.HE2010★ 22 cited

On the disappearance of broad-line region in low-luminosity active galactic nuclei: the role of the outflows from advection dominated accretion flows

Xinwu Cao

The broad-line region (BLR) disappears in many low-luminosity AGNs, the reason of which is still controversial. The BLRs in AGNs are believed to be associated with the outflows fro…

astro-ph.HE2010★ 55 cited

General relativistic polarized radiative transfer: building a dynamics-observations interface

Roman V. Shcherbakov, Lei Huang

The rising amount of polarized observations of relativistic sources requires the correct theory for proper model fitting. The equations for general relativistic (GR) polarized radi…